The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. The light distribution suggests a relatively uniform stellar population, exhibiting a gradient from a bright, yellowish core towards a less luminous, reddish outer envelope. There is little evidence of spiral arm structure or significant dust lanes. The overall shape appears somewhat elongated, leaning towards a cigar shape. There are no signs of major tidal disturbances or ongoing mergers, although some minor asymmetry may hint at past interactions.
