The galaxy appears as a moderately luminous, elliptical-like structure with a concentrated central bulge. The light distribution suggests a fairly smooth morphology, lacking prominent spiral arms or significant dust lanes. There are no major distortions of the overall galaxy shape. The object displays a moderate degree of roundness, leaning towards an in-between elliptical classification. No signs of ongoing major merger activity are immediately evident, though minor disturbances cannot be ruled out due to the image resolution. The color gradient indicates a likely mix of stellar populations, with a possibly older stellar population dominating the central bulge.
