The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellow-orange hue, suggesting an older stellar population with fewer young, hot stars and a greater proportion of red giants. The isophotes appear moderately elliptical, neither perfectly round nor highly elongated. There is some slight irregularity to the outer edges of the galaxy, possibly indicating minor disturbances or interactions. No prominent spiral arm structure is apparent in this imaging. The overall luminosity suggests a massive galaxy with a high stellar mass. There is low levels of on-going star formation. 
