The galaxy presents an overall amorphous morphology, lacking a clearly defined spiral structure. It exhibits a centrally concentrated luminosity profile, suggestive of a significant bulge component. Faint, diffuse extensions are visible surrounding the central region, indicating a possible extended halo or tidal features. The color gradient transitions from a reddish hue in the core to bluer tones in the outer regions, which might reflect differential stellar populations and ongoing star formation. The presence of irregular clumps of light suggests recent or ongoing interactions/merging activity with another galaxy, or internal disturbances affecting its overall structure. There is some slight dust lane absorption near what would be the mid-plane if it were a disc galaxy.
