The galaxy exhibits a centrally concentrated light profile, characteristic of an elliptical or lenticular galaxy. The core displays a bright, yellowish hue, potentially indicating an older stellar population. The overall shape appears largely spheroidal, though there is a slight elongation. There are subtle hints of faint, diffuse extensions, but these are not well-defined structures. No distinct spiral arms or prominent dust lanes are visible in this image. The smooth appearance of the light distribution suggests a lack of recent major mergers, though minor disturbances cannot be ruled out at this resolution.
