The galaxy presents as a primarily smooth, elliptical-like structure, with an apparent lack of distinct spiral arms or a well-defined disk. The light distribution is centrally concentrated, with a gradual decrease in luminosity towards the outer edges. The core exhibits a yellowish hue, suggestive of an older stellar population. Some very faint disk features can be seen, but it is mostly elliptical. The galaxy appears to be relatively isolated, showing no obvious signs of recent major merger activity or significant tidal distortions. There is some very minor signs of mergers/minor disturbances.
