The galaxy presents as a relatively compact, disk-shaped structure. Its color indices suggest a mixture of stellar populations, with bluer colors in the disk indicating recent or ongoing star formation activity. The disk appears fairly smooth, though some irregularities suggest possible minor disturbances. The galaxy's central region is dominated by a bright, well-defined spheroid component that is relatively round. There may be evidence of minor interaction or tidal disturbance. The luminosity suggests a galaxy with moderate stellar mass.
