The galaxy presents as a relatively smooth, elliptical morphology. There is a centrally concentrated bulge exhibiting a bright, diffuse glow. The overall shape is elongated, appearing as somewhat flattened rather than perfectly spherical. There is little evidence of prominent spiral arms or significant dust lanes. No major tidal disturbances or close companion galaxies are visually apparent, suggesting the galaxy is not currently undergoing a major merger event. There may be some minor asymmetry present, indicating possible past interactions or internal disturbances.
