The galaxy presents an overall smooth and elliptical morphology. It exhibits a concentrated central bulge that appears yellow in color, suggesting an older stellar population dominating the core. The light gradually fades moving outward from the center. The galaxy seems to be in a relatively isolated environment with no strong evidence of ongoing mergers or tidal disturbances. There is a slight elongation to the shape, but it isn't dramatically cigar-shaped. The lack of visible spiral arms or distinct dust lanes suggests that the galaxy is a relatively evolved system. Star formation appears to be subdued.
