The galaxy presents as a centrally concentrated object, generally elliptical in shape. Its core exhibits a bright, concentrated luminosity, indicative of a high stellar density. The galaxy's overall color appears to be a slightly more yellow, with subtle hints of blue in its outer regions. This color gradient potentially reflects a radial distribution in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars populating the outskirts. The galaxy's edges fade gradually into the background sky, suggesting a smooth transition in stellar density, rather than any sharply defined features. There may be the presence of low-level disturbances, but the overall symmetry suggests that it has not undergone a major recent merger event.
