The galaxy presents a generally smooth morphology, appearing largely elliptical in shape with no apparent spiral arm structures. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity moving outwards towards the galaxy's periphery. There is a subtle color gradient, with the central regions appearing more yellow/orange, suggesting an older stellar population and/or increased dust obscuration. The outer regions exhibit a bluer hue, potentially indicative of younger stars and ongoing star formation, albeit at a low rate. There's no obvious indication of any major mergers or tidal disturbances in the immediate vicinity of the galaxy, though minor disturbances cannot be ruled out given the image resolution. The galaxy displays an intermediate roundness, leaning towards being round rather than elongated or cigar-shaped.
