The galaxy presents as a slightly elongated, elliptical-like form. It exhibits a smooth, largely featureless morphology, with a dominant central bulge. The color gradient transitions from a yellowish hue in the central region to a slightly bluer periphery, indicating a possible difference in stellar populations. The galaxy appears relatively isolated, with only slight visual disturbances to its structure. Evidence suggests there may be a nearby companion, perhaps a dwarf galaxy or tidal debris. The system shows limited signs of recent or ongoing major merger activity, though potential minor disturbances could indicate past interactions. 
