The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing intensely luminous with a yellowish hue, suggestive of an older stellar population. Moving outwards from the core, the light gradually fades, and the color becomes slightly redder. The overall shape is generally round. There is little evidence of spiral arm structures or significant dust lanes. Faint, irregular features may indicate a very minor tidal disturbance. The galaxy appears relatively isolated.
