The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge with a yellowish hue, suggesting an older stellar population. There is a subtle gradient in color moving outwards from the core, with the outer regions exhibiting a slightly bluer tint, hinting at the presence of younger stars, although the overall light distribution is dominated by the older population.

There is no clear indication of spiral arm structure or significant dust lanes. The galaxy appears fairly symmetric, lacking major morphological distortions or tidal features that would suggest a recent major merger event. There's perhaps some very subtle disturbance in the outer regions on the left side of the galaxy, but this could be attributed to image artifacts. The galaxy's overall shape is roughly round.
