The galaxy appears as a moderately bright, elliptical structure. It exhibits a smooth, largely featureless morphology, with a high degree of central concentration. The light profile suggests a bulge-dominated system. The galaxy displays a yellowish-red hue in the central region, possibly indicative of an older stellar population. The outer regions are slightly bluer, potentially suggesting some on-going, but low level, star formation. There is no apparent evidence of spiral arms, a bar, or significant dust lanes. The overall shape is slightly elongated, but not strongly cigar-shaped. There is no significant evidence of tidal disturbances or ongoing mergers, though a small amount of minor disturbance cannot be ruled out. The galaxy shows an intermediate degree of roundness.
