The galaxy appears as a somewhat elliptical structure with a reddish-yellow hue. There is a slight elongation visible, indicating a deviation from a perfectly circular morphology; it is between round and cigar shaped. The central region presents a brighter intensity suggesting a concentration of stellar mass and possibly an older stellar population that are not actively forming many new stars. Faint disturbances or asymmetries can be suggested, possibly hinting at past minor interactions or internal dynamics. The galaxy is not perfectly smooth and may be exhibiting some features indicating there is still some gas present that is very slowly forming stars. 
