The galaxy presents a generally smooth, rounded morphology. Its color profile indicates the presence of both older stellar populations, exhibiting a reddish hue in the central region, and relatively younger, bluer populations towards the outer edges. The light is fairly concentrated in the center, suggesting a significant bulge component. There is faint structure at the edges, hinting that it could be a disk galaxy with arms that aren't easily seen from our angle. There are no obvious signs of ongoing major merging activity or tidal disruption. 
