The galaxy presents a generally elliptical morphology, with a relatively smooth and concentrated light distribution. A dominant central bulge is apparent, exhibiting a yellowish hue, suggestive of an older stellar population. There is a gradual falloff in surface brightness moving outward from the center, with no clear indication of spiral arms or significant star formation regions. The overall shape is slightly elongated, but broadly consistent with an elliptical galaxy classification. There is a subtle color gradient, with the central region appearing slightly redder compared to the outer regions, potentially indicating metallicity differences.
