The galaxy presents as a relatively smooth, elliptical-shaped object. The color profile indicates a predominantly older stellar population, exhibiting a yellowish hue. The light distribution is concentrated toward the center, with a gradual decrease in intensity towards the outer edges. There is no distinct evidence of spiral arms or significant dust lanes. The overall structure suggests a high degree of symmetry and a lack of major disturbances, potentially indicating a gravitationally relaxed state. A slight elongation is observed, but the galaxy appears generally rounded. There is little evidence of on-going star formation.
