The galaxy appears to be a relatively smooth, elliptical system. It exhibits a generally concentrated luminosity profile, with a slight elongation. While the overall structure suggests a lack of significant spiral arms or prominent features, there is some indication of minor disturbances or tidal features that disrupt this smoothness. 

Based on the color index, the galaxy seems to be dominated by older stellar populations, with a redder color suggesting the presence of a larger population of red giant stars and a lower rate of star formation.
