The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a predominantly round morphology with no apparent disk-like structure or spiral arms. The color profile suggests a greater concentration of older stars and a subdued amount of on-going star formation, based on its reddish-yellow hue. There is no evidence of any significant tidal disturbances or mergers in progress; the galaxy appears to be relatively isolated. The galaxy is compact, with an approximate effective radius of 4 kpc.
