The galaxy appears to be of elliptical morphology, displaying a generally smooth light distribution with a slight elongation. The central region exhibits a higher concentration of luminosity, fading gradually towards the outer edges. The light profile suggests a relatively old stellar population, with a dominant redder hue in the central region, indicative of evolved stars. There is some indication of bluer regions at the galaxy's periphery, suggestive of ongoing or recent star formation, however this is not overtly pronounced. Faint asymmetric features are present, potentially the result of a past minor merger or tidal interaction. These features may be classified as minor disturbances, and do not radically disrupt the smooth central structure. Overall, the galaxy presents as a relatively evolved system, with potential hints of recent interaction affecting its outer structure and star formation rate.
