The galaxy presents as a single, relatively compact object with a smooth, somewhat elliptical morphology. Its light distribution appears centrally concentrated, with a gradual falloff in intensity towards the outer edges. The primary color appears to be yellow-orange, suggesting a dominant population of older stars and a potentially lower rate of ongoing star formation. There is no evidence of spiral arms, a bar structure, or significant dust lanes. No tidal features or signs of recent merger activity are readily apparent, and the object appears relatively undisturbed. Overall, the galaxy is consistent with a likely elliptical galaxy at a non-negligible cosmological distance.
