The galaxy presents a largely smooth, elliptical appearance, with a concentrated central bulge. The light distribution is centrally peaked, fading gradually towards the outer regions. There is a slight elongation in the galaxy's overall shape, though it is predominantly round. Faint evidence suggests possible minor disturbances in the galaxy's structure, but no obvious signs of a major ongoing merger. The color is consistent with an older stellar population, with the light appearing redder in the central region and bluer in the extended halo. Active star formation is likely present, though it is not a dominant feature. Based on the overall morphology and color, the galaxy appears to be a relatively massive system, likely in a late stage of its evolution.
