The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a concentrated, luminous region with a yellowish-orange hue, suggestive of an older stellar population. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy appears almost perfectly round, with only a slight elongation. A faint, diffuse halo of bluer light surrounds the central region, indicating a younger stellar population beyond the bulge. No signs of major disturbances from mergers or tidal interactions are apparent. The overall color gradient suggests ongoing, but relatively low, star formation activity.
