The galaxy presents an elliptical morphology, appearing smooth and largely featureless at this resolution. The light profile suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. There's a slight elongation, trending towards a cigar shape, rather than perfectly circular isophotes. No prominent spiral arms, dust lanes, or signs of ongoing major mergers are discernible. There might be minor disturbances; however, these are difficult to assess with certainty given the image quality. The galaxy exhibits a color gradient, appearing redder in the central regions, potentially indicative of an older stellar population. The outer regions have a slightly bluer tinge, possibly indicating younger stars or lower metallicity. The overall color suggests that star formation is suppressed.
