The galaxy appears as a lenticular or early-type spiral, exhibiting a smooth, elliptical morphology. It's characterized by a bright, concentrated bulge at the center, surrounded by a more diffuse, flattened disk. The color gradient suggests an older stellar population dominating the bulge, with a yellowish or golden hue, transitioning to slightly bluer tones in the outer disk regions, possibly indicating the presence of some younger, hotter stars or ongoing star formation. There is a subtle hint of a possible dust lane or feature within the disk, but overall the galaxy presents a largely featureless appearance, hinting at a relatively quiescent history and limited current star formation activity. The light distribution suggests the galaxy is not perfectly circular, displaying a slight elongation, and is unlikely to be undergoing any major mergers, with no obvious signs of strong tidal distortions or other major disturbances.
