The galaxy presents as a fairly smooth, elliptical structure. It exhibits a concentrated central bulge which radiates strongly, suggesting a high density of stars within that region. Moving outwards from the core, the luminosity gradually decreases. There appears to be some slight asymmetry in the outer regions of the galaxy, with one side extending marginally further than the other, although overall it is well-defined.

The colour profile is relatively uniform, with a slight shift towards redder hues as you move from the outer regions inward toward the central bulge. This suggests an older stellar population dominating the core, with younger, bluer stars contributing to the outer regions, but not to a significant degree. The galaxy does not display any prominent spiral arm structures, or distinct dust lanes. 

The morphological properties suggest that it has likely undergone some minor gravitational interaction, or perhaps the early stages of a merger event in its past. The generally smooth appearance indicates that the galaxy has largely settled into a relaxed state, suggesting that any major merger events are not recent.
