The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates outward into a more diffuse halo. The color profile is dominated by yellowish hues in the core, suggestive of an older stellar population. There is a subtle gradient to redder colors in the outer regions, which are potentially indicative of even older stars or dust extinction. There is no clear evidence of spiral arm structures, prominent dust lanes, or ongoing major merger activity. Slight asymmetry could suggest a minor past disturbance, though it's nearly imperceptible. Overall, the galaxy appears to be a fairly quiescent system.
