The galaxy appears as a relatively compact and somewhat diffuse object. It exhibits a generally elliptical morphology. The light distribution appears smooth, with no obvious spiral arms or prominent dust lanes visible. The color profile suggests a dominance of older stellar populations. There is a slight elongation and asymmetry, possibly indicative of minor tidal interactions or internal disturbances. The galaxy's overall structure does not suggest it is undergoing a major merger, but smaller interactions cannot be ruled out. A central concentration of light is apparent, possibly indicating a nucleus or central bulge. Overall, the galaxy appears to be a moderately massive system with a low to moderate rate of star formation, consistent with an early-type galaxy that may have undergone some recent minor interaction.
