The galaxy appears as a relatively small, moderately bright object. It exhibits a roughly elliptical morphology, with a central bulge that is significantly brighter and more concentrated than the surrounding disk. The light distribution suggests a relatively smooth profile, although subtle deviations and irregularities are present along the edges of the disk. Faint, diffuse extensions or tidal features appear to emanate from the main body, indicative of potential gravitational interactions or past merger events. A slight asymmetry in the outer regions may suggest minor disturbances in the galactic structure. The color distribution indicates the presence of both older stellar populations in the central bulge, and younger, bluer stars in the disk region, implying ongoing or recent star formation activity. The overall appearance suggests a galaxy that has likely undergone some form of interaction or disturbance, but retains a largely intact and recognizable structure.
