The galaxy presents a generally elliptical morphology, appearing quite smooth and concentrated. A bright, prominent central bulge dominates the structure. The galaxy exhibits a color gradient, transitioning from a yellowish-white core region to a redder and fainter halo, likely indicating an older stellar population toward the galaxy's outer edges. There is a subtle hint of a surrounding disk, but it lacks the distinct spiral arms commonly observed in disk galaxies. No significant dust lanes or other features indicative of active star formation are readily apparent in the image. Minor disturbance in the morphology is possible in the outer regions.
