The galaxy exhibits a roughly elliptical morphology, appearing mostly smooth with a concentrated central bulge. The color profile indicates an older stellar population, with a yellowish hue dominating the central region, suggestive of evolved stars. There appears to be a slight asymmetry or minor perturbation in the outer regions, although a clear disk structure is not visible. Overall, the galaxy presents a generally undisturbed structure, with limited evidence of major recent or ongoing mergers. The light distribution fades gradually from the center outwards, indicating a less active star formation rate.
