The galaxy appears as a somewhat elongated, luminous object with a significant central bulge. The light profile is smooth, suggesting a relatively evolved stellar population. The galaxy's overall color is yellowish-orange, indicative of older stars and a lack of significant ongoing star formation. There is some indication of a disk component that extends beyond the central bulge, though this is less prominent. There do not appear to be any signs of recent mergers or major disturbances in the galaxy's morphology. Overall, it appears to be a relatively isolated galaxy.
