The galaxy presents as a primarily smooth, elliptical form. A slight elongation is noticeable, suggesting it may be classified somewhere between round and cigar-shaped. It displays a concentrated central bulge, brightest in the 'r' band, transitioning outwards to a fainter, diffuse halo. There are hints of subtle structures, potentially faint spiral arms or tidal features indicative of minor gravitational disturbance, however the image resolution limits any further interpretation. The galaxy exhibits a redder color profile, particularly towards the center, potentially indicating a population of older stars and lower star formation activity.
