The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The light distribution indicates a dominant bulge component, potentially indicative of an older stellar population. The overall color appears to be trending towards redder hues suggesting possible dust extinction and/or a lack of significant ongoing star formation. There are hints of faint, diffuse extensions or a very subtle disk-like structure surrounding the central bulge, but the resolution limits a definitive classification. No obvious signs of major mergers or tidal disturbances are visible within the immediate vicinity of the galaxy. The galaxy displays a generally undisturbed morphology.
