The galaxy presents as a centrally concentrated object with a smooth light profile, suggesting a relatively old stellar population. It appears to be an elliptical or lenticular galaxy, exhibiting a somewhat flattened shape but lacking the distinct spiral arm structures characteristic of spiral galaxies. The central bulge is luminous and dominates the overall brightness. There is a subtle color gradient apparent, transitioning from a yellower core region to a slightly bluer halo. This indicates potential variations in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars possibly residing in the outer regions. There is no evidence of significant ongoing star formation regions or prominent dust lanes. The overall structure seems undisturbed, showing no signs of recent major mergers or tidal interactions. Any merger events or accretion history is likely in the past, as the system appears relaxed and morphologically smooth.
