The galaxy presents as a relatively compact object with an elliptical morphology. There appears to be little to no resolved substructure, such as spiral arms or prominent dust lanes, visible in this image. The light distribution suggests a smooth and centrally concentrated stellar population. The shape appears elongated, deviating significantly from a perfect circle, and possesses a cigar-like structure. Given its red color, the galaxy is likely composed primarily of older stars, indicating a relatively low rate of on-going star formation. There are no signs of major tidal features or obvious disturbances indicative of an advanced merger event, though some subtle morphological irregularities cannot be ruled out. Overall, this appears to be a quiescent elliptical galaxy.
