The galaxy presents a largely smooth and rounded morphology. A dominant, centrally concentrated bulge is apparent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The galaxy lacks a prominent spiral arm structure or distinct features indicative of ongoing major mergers. Faint extensions or minor irregularities are barely visible, possibly indicating a subtle interaction or past disturbance. Overall, the galaxy appears as an elliptical galaxy, possibly of type E4-E5. Further analysis of the light profile and detailed spectral properties are necessary to ascertain the precise star formation history and dynamics within this galaxy.
