The galaxy presents as a relatively smooth, elongated structure, likely an elliptical galaxy. Its core exhibits a concentrated, bright luminosity, suggesting a high density of stars in the galactic center. The luminosity gradually decreases outwards from the center, forming a diffuse halo. The galaxy displays a subtle color gradient, transitioning from a yellowish-white core to a bluer outer region. There is no apparent spiral arm structure or dust lane visible. Faint asymmetries on the outer edge are possibly signs of tidal disturbances, though they could be internal structures. The galaxy's shape is moderately elongated, classified as somewhere between round and cigar-shaped. There are no signs of any ongoing major merger events or significant disturbances in the overall morphology, however, there are signs of minor disturbances or a prior merger event.
