The galaxy presents a generally elliptical morphology. It appears to be relatively smooth in structure, lacking prominent spiral arms or significant dust lanes visible in this image. The central bulge appears bright and concentrated, exhibiting a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy are less luminous and have a slightly bluer tint, possibly indicating the presence of some younger stars or ongoing star formation, albeit at a low rate. The elongated shape suggests that it is either a highly elliptical galaxy, or a spiral galaxy viewed at an angle, but the lack of defined spiral arms suggests the former is more likely. There is no indication of a recent merger or major disturbance, based on the smooth, regular shape and the lack of tidal tails or other debris.
