The galaxy presents as an elliptical morphology, appearing generally smooth with a concentrated central bulge. There are no obvious spiral arm structures or distinct dust lanes visible in this image. The color profile indicates a redder central region, possibly indicative of an older stellar population and a lower rate of ongoing star formation. The outer regions exhibit a bluer hue, suggesting the presence of some younger stars. Overall, the galaxy appears relatively undisturbed, with no clear signs of recent mergers or significant tidal interactions. The shape is close to round, with only a slight deviation toward an elongated or cigar-like appearance.
