The galaxy presents as a relatively smooth, elongated structure. Its morphology is suggestive of a lenticular or possibly an elliptical galaxy, exhibiting a notable lack of prominent spiral arms. The luminosity profile appears concentrated towards the center, with a gradual decline in brightness towards the outer regions. The color gradient indicates a redder hue in the central bulge, potentially indicative of an older stellar population, while the outer regions exhibit a slightly bluer tint, hinting at the presence of younger stars, though this is less pronounced. There is no obvious evidence of ongoing major mergers or tidal disturbances, suggesting the galaxy is relatively settled. Faint, diffuse features may be present, though their nature is difficult to discern without higher resolution data. The overall structure is subtly asymmetric, with a slight elongation along its major axis. The size of the galaxy appears moderate. Overall the galaxy appears to be old with a low star formation rate.
