The galaxy presents as a relatively compact, elongated structure. Its overall color appears to be a yellowish-white, potentially indicating an older stellar population. The central region is brighter and more concentrated, suggesting a higher density of stars there. There are signs of slight asymmetry or disturbance, possibly hints of interactions with another galaxy, although the bulk of the light emanates from a centrally located source. Some faint extensions or tidal features appear, indicating possible gravitational disturbances. These possible signs of merging appear in the form of faint plumes. There is no obvious spiral structure. 
