The galaxy presents a generally smooth, elliptical morphology. It exhibits a slightly elongated shape, appearing more "in-between" round and cigar-shaped. There is a distinct central bulge that appears redder in color, suggesting an older stellar population. The surrounding disk is bluer, possibly indicating ongoing star formation, although at a low rate. There is evidence of minor disturbances in the galaxy's structure, which could indicate tidal interactions or a past minor merger event. There are no obvious spiral arms or a strong bar structure visible.
