The galaxy presents as a generally smooth, elliptical-like object with a concentrated central bulge. The light appears to be dominated by older stellar populations, indicated by the yellowish-red hue of the bulge, suggesting less active star formation. There is very little evidence of spiral arm structure or dust lanes, consistent with a relatively undisturbed morphology. The outskirts appear diffuse, gradually fading into the background sky. Overall, the galaxy exhibits characteristics of a mature galaxy with potentially suppressed star formation. The general shape is closer to in between round and cigar shaped. There are no signs of significant merging or tidal disturbances.
