The galaxy presents as a primarily smooth structure, exhibiting an elliptical morphology. The central region displays a high concentration of luminosity, appearing significantly brighter and more concentrated than the surrounding area. There appears to be a subtle color gradient, shifting from yellow-white towards the core to a slightly redder hue at the outer edges, suggesting possible variations in stellar populations or dust content. The galaxy's overall form suggests a system dominated by older stellar populations and a relatively low rate of current star formation. There is a very slight hint of a disk-like structure, possibly representing a weak disk component, but the smoothness of the overall appearance predominates. The shape is largely ellipsoidal but it does deviate slightly from a perfect circle, suggesting a slightly elongated appearance but not highly cigar shaped. There do not appear to be any major distortions or tidal features, and the object seems fairly isolated with no obvious signs of recent or ongoing merger activity.
