The galaxy appears to be a relatively smooth, elliptical-type galaxy. The central region exhibits a concentrated, bright core, surrounded by a more diffuse, extended halo. The galaxy has a yellowish-red hue, suggestive of an older stellar population with a low rate of ongoing star formation. There is a slight asymmetry to the galaxy's light distribution, possibly indicating a minor interaction or disturbance. The galaxy presents a generally rounded morphology, with a slight deviation towards an elongated, cigar-like shape. The overall structure seems mostly undisturbed, with no obvious signs of major merging activity. 
