The galaxy presents a roughly elliptical morphology, with a relatively smooth, concentrated central bulge that dominates the overall structure. The bulge exhibits a bright, unresolved core, suggesting a high stellar density or potential active galactic nucleus. Surrounding the bulge is a fainter, more diffuse halo or disk component. There is subtle indication of some structure within the disk, hinting at spiral arm morphology, but these are not well-defined. The overall color of the galaxy appears to be slightly redder in the central regions, possibly indicating an older stellar population, with bluer colors more apparent in the outer regions, potentially due to ongoing star formation. The galaxy shows no obvious signs of significant tidal disruption or major mergers.
