The galaxy presents as a relatively compact object with a smooth, elliptical morphology. It appears to be a spheroid-dominated system with minimal visible dust lanes or spiral arm structures. The color gradient suggests an older stellar population, displaying a yellowish-red hue towards the galactic center, possibly indicative of a concentration of evolved stars. There is a subtle bluer component within the galaxy, but it is not very pronounced. There might be a slight distortion visible which could indicate a past or ongoing minor merger event, or the presence of a faint, unresolved tidal tail. This is not definitive.
