The galaxy presents as a somewhat elliptical, disk-like structure with a bright, concentrated central bulge. The disk appears relatively smooth in texture, with no apparent spiral arm structures visible. The color gradient transitions from a bluer hue towards the central regions to a yellower tone in the outer regions, possibly indicating different stellar populations and ongoing star formation. The galaxy is moderately inclined relative to our line of sight. The absence of significant dust lanes or prominent star-forming regions suggests the galaxy is an intermediate stage in its evolutionary path or is a more evolved system. The overall morphology implies a galaxy with a moderate degree of flattening and rotational support.
