The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears to be a relatively older stellar population given its yellowish-orange hue, suggesting lower levels of current star formation. The radial light profile decreases smoothly from the core outward, indicating minimal substructure or spiral arm features. There is little evidence of recent major mergers or tidal disturbances in this image. A very slight elongation is observed, but the galaxy approximates a spheroid. The colors suggest it is a relatively massive system. The observed size is consistent with a typical galaxy at its distance.