The galaxy presents as an elongated, elliptical structure with a smooth, featureless morphology. The light distribution shows a concentrated, bright central region that gradually fades towards the outer edges. The major axis is significantly longer than the minor axis, giving it a cigar-like appearance. The galaxy exhibits a blueish-white hue centrally, suggesting the presence of some younger stellar populations and ongoing, albeit low, star formation. The faint outer regions appear redder in comparison, potentially indicating older, cooler stars. There is no discernible spiral arm structure or obvious dust lanes. The overall impression is that of a relatively undisturbed, low-mass system with an aging stellar population.
