The galaxy presents a slightly inclined disk-like structure with a prominent central bulge. The bulge region exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter, bluish-white diffuse arms extend from the central bulge. The overall form of the galaxy is neither perfectly smooth nor displaying grand spiral arm structures, exhibiting some irregularities. There may be faint evidence of some form of tidal interaction in the form of a slight asymmetry or distortion in the outer disk. The galaxy appears to be neither a pure elliptical nor a well-defined spiral; it could be an intermediate type, possibly in the process of some merging or interaction event. Star formation appears to be present within the disk, indicated by the bluer color.
