The galaxy appears as a centrally concentrated, roughly elliptical object. It exhibits a smooth, diffuse profile with no readily discernible spiral arm structure or prominent dust lanes. A subtle color gradient is observed, with a slightly yellower hue towards the galactic center, suggesting an older stellar population concentrated there. The outer regions display a bluer tint, potentially indicating the presence of younger stars, but the resolution is insufficient to confirm the presence of individual star-forming regions. The galaxy's overall structure suggests a relatively relaxed dynamical state, with no obvious signs of ongoing major mergers or significant tidal disturbances. The observed morphology is consistent with an early-type galaxy, possibly an elliptical or lenticular type.
