The galaxy presents as a primarily smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing elongated with an axis ratio suggesting a moderate degree of flattening. There is a subtle color gradient across the galaxy's surface, with the core region displaying a slightly bluer hue compared to the redder outer regions. This suggests a population of younger, hotter stars concentrated towards the center, though the dominant stellar population appears to be older and redder. No spiral arm structures or prominent dust lanes are discernible. There is no evidence of any major ongoing merger activity or significant tidal disturbances. A very subtle, diffuse halo may be present, extending slightly beyond the main body of the galaxy. The galaxy displays a moderate redshift, indicating it is at a significant cosmological distance.
