The galaxy appears to be a relatively smooth, disk-shaped galaxy with a noticeable central bulge. The color profile suggests a concentration of older stars in the bulge, indicated by the yellowish-white hue, and bluer stars tracing the disk, possibly implying ongoing star formation. The galaxy exhibits a slight ellipticity, suggesting it is being viewed at an angle relative to its rotational axis. There is no apparent major disturbance, tidal tails, or merging companion. The galaxy seems relatively isolated, with no obvious interacting neighbors in the immediate vicinity. The light distribution follows a generally smooth profile, indicative of an earlier-type spiral or a lenticular galaxy.
