The galaxy presents as a roughly circular, unresolved object. Its core region exhibits a bright, concentrated luminosity, suggesting a high density of stars and possibly a supermassive black hole actively accreting material. The galaxy appears quite smooth, with no readily discernible spiral arms or prominent dust lanes. A slight color gradient is observed, transitioning from a bluer hue near the center to redder tones in the outer regions. This could indicate a population of younger, hotter stars in the central area and older, cooler stars further out, or differential dust extinction. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy.
