The galaxy presents as a relatively smooth, elliptical morphology. Its light profile is concentrated towards the center with a gradual decline in surface brightness outwards. The core region exhibits a yellow-orange hue, suggestive of an older stellar population, with diminishing blue light. The overall shape is slightly elongated. There is no apparent spiral structure or significant dust lane obscuration. The galaxy appears isolated, showing no clear signs of interaction or tidal disturbance in this image.
