The galaxy presents a generally smooth, elongated morphology. It exhibits a central bulge, with a moderately defined structure. The bulge appears to have a slightly yellowish tinge, possibly indicating an older stellar population. Extending from the bulge is what looks to be a disturbed disk that could be described as being somewhat cigar-shaped. The disk exhibits a bluer color gradient, suggestive of ongoing or recent star formation. This bluer light is less pronounced closer to the central bulge and appears to be more prominent further down the length of the disk. There is some asymmetry in the outer regions of the disk. There are no apparent spiral arm structures within the galaxy, though there may be some dust obscuring the structure of the disk. The object appears to have little ongoing star formation, possibly indicating a late-stage spiral galaxy transitioning to a more quiescent state. There may be minor disturbances or tidal features, that could be indicative of minor gravitational interaction with another galaxy.
