The galaxy presents as a relatively smooth, elongated structure. Its morphology appears largely elliptical, with a noticeable central bulge. The color gradient suggests a concentration of older stellar populations in the core, shifting towards bluer hues in the outer regions, though this is subtle. There's no obvious spiral arm structure detectable within the resolution of this image, nor is there a clear presence of ongoing major mergers or tidal distortions. Minor disturbances may be present, but not clearly. The galaxy's shape is not perfectly round; it displays an intermediate ellipticity, closer to cigar-shaped than circular. The galaxy is not exceptionally bright, with moderate star formation, if any.
