The galaxy presents as a somewhat elongated, elliptical structure with a bright, concentrated central bulge. The galaxy exhibits a smooth, diffuse light distribution, with no distinct spiral arms or prominent dust lanes visible. There appears to be a slight color gradient, with the central region appearing more yellow/orange, suggesting an older stellar population and less ongoing star formation within the nucleus. The outer regions seem slightly bluer, hinting at the presence of younger stars or a low level of star formation activity in the galaxy's outskirts, but there is no star forming region evident. It does not appear to be undergoing a major merger.
