The galaxy presents as a well-defined elliptical or lenticular structure. The light profile appears smooth and concentrated towards the center, indicating an older stellar population. The galaxy exhibits a dominant yellowish hue, possibly signifying a lack of significant ongoing star formation and the presence of evolved stars. The overall shape is elongated, but not extremely so; it appears to be somewhere in between a perfect circle and a cigar shape. There is no apparent major disturbance or signs of a recent major merger event. Indications suggest potential minor disturbances or tidal interactions, though not overtly apparent.
