The galaxy presents a generally smooth, rounded morphology. It exhibits a concentrated central bulge that gradually diffuses outwards. The light distribution is centrally peaked, indicative of a possible elliptical or S0 classification. There is no discernible evidence of spiral arms or significant dust lanes. The galaxy has a yellowish-white hue, potentially indicating an older stellar population with lower ongoing star formation activity. There is no apparent signs of any major disturbances or merging events. Overall, the galaxy appears to be a relatively quiescent, well-formed structure.
