The galaxy presents as a somewhat smooth, elliptical-like structure. It appears to have a central bulge that is notably brighter and more concentrated than its outer regions. The overall shape is elongated, suggesting a moderate degree of ellipticity, potentially resembling an E4-E6 type galaxy based on the Hubble sequence. There is a slight hint of a disk but the bulge dominates the appearance. The color profile shows a predominantly red-yellow hue. This color suggests an older stellar population, with a lower rate of ongoing star formation. No significant dust lanes or prominent spiral arms are visible. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or interactions.
