The galaxy appears to be a relatively smooth, elliptical or lenticular system, exhibiting a centrally concentrated morphology. It is somewhat elongated, displaying a moderate deviation from a perfectly circular shape, hinting at a possible cigar-shaped structure. There may be a slight asymmetry in the light distribution, with a subtle extension or tidal feature on one side. The galaxy's light profile is relatively diffuse, lacking prominent spiral arms or distinct features typically associated with actively star-forming galaxies. There is a noticeable lack of intense blue light indicative of ongoing star formation; its overall color suggests an older stellar population. No significant signs of a major merger or strong tidal interactions are evident, however some form of minor disturbances cannot be ruled out. The galaxy displays an overall smooth appearance.
