The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The color profile is dominated by yellow-red hues, indicative of an older stellar population with a relatively low rate of recent star formation. The galaxy exhibits a slight elongation, appearing neither perfectly spherical nor highly flattened. There's minimal evidence of spiral arm structures or significant dust lanes within the observed region, and no indications of ongoing or recent major merger events. Subtle disturbances may be present, however no strong merging or tidal tails are apparent.