The galaxy presents as an elongated, disk-like structure, viewed at a steep inclination, close to edge-on. The central bulge is visibly prominent, exhibiting a concentrated brightness and a yellowish-white hue, indicative of an older stellar population. Moving outward from the bulge toward the edges, a gradual transition to a bluer color is observed. The disk appears relatively smooth, with faint signs of structural features such as spiral arm segments or dust lanes, but these are not sharply defined, likely due to its steep inclination and relatively small size. There is no apparent evidence of a major ongoing merger, however, there may be some minor tidal disturbance.
