The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. The isophotes are generally round, although there appears to be a slight asymmetry in the outer regions, possibly indicating a minor gravitational interaction or past merger event, but not enough to disrupt the overall smoothness. The color profile appears to be red, with the central regions trending yellow, implying an older stellar population with suppressed recent star formation. There are faint signs of a possible disk-like component, though the structure is dominated by the smooth spheroid.
