The galaxy appears to be a relatively smooth, centrally concentrated object with an elliptical morphology. Its light profile exhibits a gradual decline in intensity from the core outwards. The central region displays a yellowish-orange hue, suggestive of an older stellar population. Surrounding the core, there's a broader, less intense halo of bluish light, potentially indicating some ongoing, though limited, star formation activity. No distinct spiral arms or bar structures are discernible. The overall shape appears close to round, with minimal elongation or asymmetry. There is no obvious evidence of a major merger or tidal disturbances, though some subtle irregularities in the outer regions cannot be completely ruled out, and could indicate a minor interaction in its past.
