The galaxy presents as an elliptical structure with a smooth, diffuse light distribution. A concentrated, bright central bulge is noticeable, exhibiting a yellowish hue, potentially indicating an older stellar population. Fainter, bluer regions are observed extending outwards from the core along the galaxy's major axis, suggesting ongoing star formation. While the image resolution is limited, there is a subtle hint of a disk-like structure. There are no immediately obvious signs of strong tidal disturbances or major mergers, though the presence of the bluer regions might indicate minor interactions or internal processes affecting star formation. The galaxy's overall shape leans towards an intermediate roundedness rather than a perfectly circular or elongated form.
