The galaxy presents a morphology consistent with a spiral or lenticular type. It displays a bright, centrally concentrated bulge, suggesting a significant population of older stars. Surrounding the bulge, a relatively smooth, diffuse disk is visible, exhibiting a subtle blue hue towards the outer edges which could indicate some ongoing star formation. The overall shape is somewhat elongated, appearing more "in-between" round and cigar-shaped, possibly indicative of a slight inclination relative to our line of sight. There are no obvious signs of strong tidal interactions or major disturbances, though faint asymmetrical features within the disk might suggest minor disturbances or past interactions.
