The galaxy presents as a centrally concentrated object with a somewhat amorphous structure. While a clear disk is not immediately apparent, the galaxy exhibits features that deviate from a perfectly smooth elliptical morphology. Faint hints of a disk-like structure or spiral arms may be present, though the overall light distribution appears relatively uniform. There is some indication of possible minor disturbances in the morphology, perhaps due to a small interaction or tidal feature on one side. The galaxy's color gradient suggests a relatively even distribution of stellar populations, with a tendency towards redder hues in the central region and bluer hues in the surrounding regions. There may be a subtle, faint halo surrounding the central body of the galaxy. Overall, the galaxy appears as a transition object between a purely elliptical galaxy and a more structured spiral system, with signs of possible past or ongoing interactions.
