The galaxy presents as a somewhat elliptical, lenticular structure, appearing largely featureless. A bright, concentrated nucleus dominates the galaxy's central region, with the luminosity gradually decreasing outwards. There is a faint, extended halo or disk surrounding the central bulge. The color profile indicates an older stellar population, with a yellowish-red hue concentrated in the central regions and a slightly bluer tint in the outer regions, indicative of potentially younger stars. There's a hint of minor asymmetry in the outer halo, possibly suggesting a past or ongoing minor interaction or disturbance. Overall, the galaxy exhibits characteristics consistent with a relatively evolved system undergoing little active star formation.
