The galaxy presents as a somewhat amorphous, elliptical object with a smooth appearance. Its light profile suggests a relatively uniform distribution of stars, with a slightly brighter, more concentrated central region, likely indicating the presence of a bulge. There is a slight elongation, deviating from a perfectly spherical shape, perhaps indicating a minor interaction or recent accretion event. Color variations suggest varying stellar populations, with a yellowish-orange hue dominating the central area, potentially indicative of older, redder stars. Fainter, bluer tinges are visible in the outer regions, hinting at some ongoing, albeit low level, star formation. There appear to be faint disturbances in the outer arms as well. These disturbances could also be the result of dust absorption. Overall, it appears to be a massive galaxy, relatively quiescent in terms of star formation activity.
