The galaxy presents a largely smooth morphology, appearing as a single, relatively featureless entity. It displays a centrally concentrated luminosity profile, with brightness decreasing radially from the core. The overall shape leans towards a round form, with subtle deviations giving it a somewhat elliptical appearance. The galaxy's color index suggests the presence of a predominantly older stellar population, with a visible contribution from bluer, potentially younger stars, towards the outer regions. There is no indication of significant ongoing major mergers or tidal disturbances, however minor disturbances cannot be ruled out. Given the luminosity and apparent size, the galaxy is consistent with being a massive system at a considerable cosmological distance.
