The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge. The light profile appears to gradually decrease from the center outwards. The galaxy exhibits a subtle color gradient, with the core appearing more yellowish, suggesting an older stellar population dominating the central region. The outer regions show a faint bluish tint, which could indicate the presence of some younger, hotter stars, although it does not appear to be highly significant. There are no obvious spiral arm structures or prominent dust lanes visible in this image. There might be minor disturbances within the galactic structure. The overall shape appears somewhat elongated but not drastically so. The galaxy's light is brightest in the redder wavelengths with less bright blue light. The estimated mass of the galaxy suggests it is a fairly large system, and that it is forming new stars.
