The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a concentrated, bright, yellowish-orange hue, suggesting a substantial population of older stars. A fainter, reddish-orange extension is visible to the left, potentially indicative of a tidal feature or a smaller merging galaxy. The overall form is somewhat irregular, deviating from a perfect ellipse, possibly disturbed by gravitational interactions. No obvious spiral arm structure is discernible. There is an absence of noticeable dust lanes within the galaxy, supporting its classification as a relatively quiescent system.
