The galaxy appears as a somewhat flattened, elliptical structure, with a smooth, diffuse light distribution. The central region exhibits a higher concentration of yellow-orange light, suggesting an older stellar population. Fainter and bluer light is also present. The shape of the galaxy can be described as in between round and cigar shaped. There is a suggestion of a possible minor disturbance or interaction on one side of the galaxy, given the blue light. There is no significant structure detected within the galaxy, such as spiral arms or dust lanes. The galaxy appears relatively isolated with no signs of a major merger, although the shape could suggest a previous interaction. Based on the color and smoothness, the galaxy is likely a fairly massive system, with an intermediate star formation rate.
