The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates outward into a more diffuse halo. The galaxy's overall color profile appears generally redder, particularly in the core, suggesting an older stellar population. Faint blueish irregular features are visible in the outer regions, potentially indicating areas of more recent, albeit subdued, star formation. There is no strong evidence of spiral arm structures or a prominent disk. A slight elongation is observable, deviating from a perfectly circular shape, but it is not distinctly cigar-shaped. There are no obvious signs of major mergers or significant tidal disturbances, although a slight asymmetry may suggest past minor interactions. The galaxy appears well-defined, without substantial artifacts impacting its visual characteristics.
