The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests an elliptical morphology, with a high degree of radial symmetry and minimal evidence of spiral arms or a disk structure. There is a slight elongation in its shape, though it appears mostly rounded. The galaxy's color profile indicates a moderate stellar population age, with a mix of older, redder stars concentrated in the core and slightly younger, bluer populations extending outwards. The light is dominated by yellowish hues, suggesting a lack of significant ongoing star formation. There is no clear indication of tidal features, strong dust lanes, or other signs of recent major mergers or interactions. Minor disturbances may be present but not easily discernable. Overall, it appears to be a relatively quiescent, evolved galaxy.
