The galaxy presents as a predominantly smooth, elliptical structure. It exhibits a radial color gradient, transitioning from a concentrated yellowish-white core to a fainter, reddish-hued outer region. There is little evidence of spiral arm structure or significant dust lanes. The overall shape appears relatively round, with only a slight deviation toward an elongated form. No obvious signs of recent major mergers or tidal disturbances are discernible, although subtle asymmetries or minor disturbances cannot be ruled out at this resolution. The galaxy's color suggests a population dominated by older stars, with relatively low ongoing star formation.
