The galaxy presents a largely elliptical morphology. It appears quite smooth and concentrated, with a bright, unresolved core suggestive of a significant central bulge. There is little evidence of spiral arm structure or distinct dust lanes. The color profile indicates a generally older stellar population, trending towards redder hues in the central regions and slightly bluer towards the outer edges. The lack of significant morphological distortions suggests it is not currently undergoing a major merger event, though the slight irregularities in its outer halo could point to minor interactions or past accretion events. Based on its overall appearance, this is likely a massive galaxy.
