The galaxy appears to be a spiral galaxy, likely seen at a moderately oblique angle, with a notable central bulge. The bulge exhibits a yellowish-white hue, which may indicate an older stellar population. Fainter spiral arms extend from the bulge. These arms appear somewhat patchy, displaying a bluer tint in places, potentially signifying regions of more recent star formation. The galaxy possesses a disk that is relatively well-defined, although it seems slightly perturbed or distorted, showing some faint tidal features which may be indicative of past or ongoing interactions or mergers. Overall, the galaxy does not appear to be undergoing vigorous star formation.
