The galaxy presents as an elliptical morphology with a smooth, largely featureless light distribution. It exhibits a centrally concentrated luminosity profile, with the brightness decreasing gradually outwards. The galaxy appears moderately rounded, showing only a slight elongation. There is a hint of a disk structure that could be present, but that is not significant.

In terms of color, the core region is a blend of colors, appearing more blue shifted, suggesting the presence of a younger stellar population or active star formation. The outer regions have a redder hue, potentially indicating an older stellar population and minimal ongoing star formation. No major disturbances or tidal features are visually apparent, suggesting that the galaxy has not undergone a major merger event in the recent past.

Based on the overall characteristics, this galaxy appears to be an early-type elliptical galaxy, displaying evidence of a past merger event that has settled into a quiescent, spheroidal structure.
