The galaxy presents a smooth, elliptical morphology. Its overall shape appears cigar-like, with a significant departure from circular symmetry. The light distribution suggests a centrally concentrated stellar population, gradually fading toward the outer regions. There is no obvious evidence of spiral arms or significant dust lanes. The galaxy exhibits a relatively homogenous color profile, trending towards redder hues, potentially indicative of an older stellar population. No signs of major mergers or tidal disturbances are readily apparent.
