The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears concentrated towards the center, with a bright, yellowish core indicative of an older stellar population. There's a subtle color gradient moving outward from the center towards a slightly bluer hue, hinting at the presence of some younger stars on the outskirts, although the galaxy is predominantly composed of older stars. No distinct spiral arms or significant dust lanes are visible. There appear to be no signs of ongoing or recent major mergers or tidal interactions. The galaxy exhibits a generally rounded shape with only slight deviations from perfect circularity. It appears to be a fairly isolated elliptical galaxy.
