The galaxy presents as a somewhat diffuse and luminous object. It exhibits an overall smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The light distribution appears centrally concentrated, suggesting a prominent bulge component. The galaxy exhibits a generally rounded appearance. There are faint hints of possible minor disturbances or tidal features in the outskirts, but no clear evidence of a major merger or strong interaction. Color gradients appear to be subtle across the galaxy's body. The overall color profile leans towards the redder end of the spectrum, indicative of an older stellar population.
