The galaxy exhibits a roughly elliptical morphology, appearing mostly smooth with a concentrated central bulge. There is some indication of faint, extended structure surrounding the main body, although the image resolution limits detailed analysis of this feature. Color gradients suggest a possible radial variation in stellar populations or dust distribution within the galaxy. The core appears bright, possibly due to ongoing star formation. There is no visually obvious presence of spiral arms or a prominent disk structure. The galaxy does not seem to be strongly interacting with any nearby companions, and there is no visible morphological evidence for a recent major merger.
