The galaxy presents a generally elliptical morphology, appearing somewhat elongated. Its central region exhibits a concentrated luminosity, suggesting a significant stellar population. The light from this central bulge is yellowish, likely indicative of older stars. The outer regions show a fainter, more diffuse structure, with some areas of bluish light suggesting younger stellar populations and ongoing star formation. A small region on the outskirts displays a reddish hue, potentially caused by dust obscuration or a region of intense star formation within dust clouds. The galaxy appears relatively undisturbed, showing no strong signs of a recent major merger, though some asymmetry suggests minor disturbances may have occurred. Overall, it seems to be an evolved galaxy with both old and new star formation regions.
