The galaxy presents as a somewhat elliptical structure, with a smooth, diffuse appearance. A concentrated central bulge is visible, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer tint, implying the presence of younger, hotter stars. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions, although a subtle asymmetry or minor disturbance cannot be ruled out. There may be faint spiral arm segments that cannot be clearly distinguished due to the galaxy's morphology and image resolution. The galaxy does not appear to be perfectly round but rather has an elongated, cigar-like shape, which could indicate it is in the process of transforming from a spiral to an elliptical galaxy. The overall color suggests that star formation is occurring at a slow rate.
