The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely rounded in shape. The color profile suggests a somewhat evolved stellar population, with a yellowish-white core transitioning to slightly bluer hues in the outer regions, potentially indicating some ongoing or recent star formation activity. There are no distinct spiral arms, bars, or other prominent features readily apparent in the disk, suggesting a system dominated by a spheroid component. No significant tidal distortions or interactions with other galaxies are evident, though there may be a faint possible sign of a minor disturbance in the galaxy's disk.
