The galaxy presents a generally smooth morphology, appearing elliptical in shape. The light is concentrated toward the center, indicative of a significant bulge component. There's a subtle color gradient, with the central regions appearing more yellow/red, possibly indicating an older stellar population and less active star formation in the core. Fainter, bluer light is discernible in the outer regions, suggesting the presence of some younger stars or ongoing star formation, though at a lower rate than in actively star-forming galaxies. There are no distinct spiral arms or prominent dust lanes visible, supporting the classification as an elliptical galaxy. No signs of major mergers or tidal disturbances are immediately apparent. The overall appearance suggests a relatively evolved system.
