The galaxy presents a largely smooth morphology, appearing elliptical or lenticular in nature. It exhibits a notable concentration of light toward the galactic center, with a gradual decrease in luminosity outward. There is a subtle color gradient, transitioning from a slightly more yellow-red hue in the core to a subtly bluer tint in the outer regions. The overall shape tends to be relatively round. There is no evidence of strong tidal interactions or significant morphological disturbances, although the presence of very faint features in the surrounding area cannot be entirely ruled out without further analysis. The galaxy's color profile suggests an evolved stellar population, but some level of ongoing, albeit low, star formation activity may be occurring.
