The galaxy presents as a largely featureless spheroid. It exhibits a smooth, centrally concentrated luminosity profile. There is minimal evidence of spiral arms or a significant disk component. Coloration suggests a relatively older stellar population, with a slightly higher concentration of bluer light at the core, possibly indicating a region of ongoing, albeit subdued, star formation. The galaxy's shape is closer to elliptical, with only a slight deviation from perfect circularity. There is no indication of any major ongoing mergers or significant tidal disturbances in the immediate vicinity, although subtle asymmetries may hint at minor past interactions.
