This galaxy presents as a relatively smooth, lenticular-like structure. It exhibits an elliptical morphology, with a slight elongation visible along one axis. The central region displays a concentrated luminosity, suggesting a prominent galactic nucleus. The color profile indicates a primarily older stellar population, with a reddish-orange hue dominating the core, transitioning to a more subdued blueish color in the outer regions. This color gradient hints at potential ongoing or recent, but low levels, star formation activity in the disk. There is no distinct dust lane or spiral arm structure discernible in this image. A slight asymmetry is noted in the distribution of light in the outer regions of the galaxy, which may point to possible past minor merger events or tidal disturbances, but this is unconfirmed. The overall appearance suggests a relatively evolved galaxy transitioning away from active star formation and towards a more quiescent state.
