The galaxy presents as a single, concentrated body, suggestive of an elliptical or lenticular morphology. It exhibits a smooth, centrally concentrated luminosity profile, with the light intensity decreasing gradually outward from the core.

The dominant color is a soft yellow-white, potentially indicating an older stellar population and a lack of significant ongoing star formation across the galaxy as a whole. However, there is evidence of faint blue-green light in the lower portion of the galaxy, which could indicate localized regions of more recent star formation. Additionally, there appears to be some dust in the same location, which may be correlated with the area of star formation. The galaxy exhibits a slight ellipticity.
