The galaxy presents as a relatively smooth, elliptical morphology with minimal discernible features. It exhibits a concentrated central bulge that gradually diffuses outwards. The color profile suggests a generally older stellar population, dominated by redder hues. There is little evidence of active star formation, as indicated by the absence of significant blue or ultraviolet light emission. The galaxy appears relatively isolated, showing no strong tidal interactions or significant disturbances in its morphology. The galaxy's overall structure is consistent with a spheroid-dominated system, potentially a massive early-type galaxy.
