The galaxy presents a primarily smooth and diffuse appearance, suggesting it may be an elliptical or lenticular type galaxy. It exhibits a centrally concentrated bulge that fades gradually into the outer regions, lacking prominent spiral arms or distinct features. The overall color appears to be relatively uniform, with a slight bluish tint. This hints at the presence of a population of younger, hotter stars, though this is subtle, and the galaxy might also consist of mostly older stars. The galaxy's shape is somewhat elongated, possibly indicating a degree of rotation or a recent merger event, though no major disturbances are visible in this single image. There is a lack of visible dust lanes or patchy star forming regions, further reinforcing the impression of a well-mixed stellar population.
