The galaxy presents as a centrally concentrated, relatively smooth system with a primarily elliptical morphology. A slight elongation is discernible. The central region exhibits a yellowish hue, suggestive of an older stellar population dominating the core. Moving outwards from the core, the color transitions to a bluer tinge, suggesting the presence of a younger, star-forming population, but this is not the dominant color. No distinct spiral arm structures or dust lanes are immediately obvious. Based on the smooth appearance, it is most likely a galaxy that has undergone significant merging activity in its past, resulting in a relatively homogenous stellar distribution. Evident in the image are some signs of mild disturbance.
