The galaxy presents a generally smooth appearance with a notable absence of defined spiral arms or a prominent disk. The light distribution suggests an elliptical morphology, elongated along a major axis. Color gradients within the galaxy indicate a redder central region, potentially indicative of an older stellar population, with a gradual shift towards bluer hues in the outer regions. The overall structure appears undisturbed, with no obvious signs of tidal interactions or major mergers. The integrated color profile points towards ongoing star formation, albeit at a modest rate. The galaxy's light is moderately concentrated.
