The galaxy presents a largely smooth and rounded morphology. There is a central concentration of light, possibly indicative of a bulge. No distinct spiral arms or bar structures are discernible. The overall color is a pale bluish-white, potentially suggesting a mix of stellar populations. There is little evidence of ongoing major merging activity or significant tidal disturbances. The galaxy appears relatively isolated with no nearby companions. Faint, diffuse emission extends outwards from the central region. It may be an elliptical galaxy.