The galaxy presents as a concentrated spheroid of light, approximately circular in projection. The core exhibits a high surface brightness, with the light intensity gradually decreasing towards the outer regions. The color of the core appears slightly yellow/white, suggesting an older stellar population dominating the central region. There is no evidence of spiral arm structure or a prominent disk. The overall smooth appearance indicates a high likelihood of being an elliptical galaxy with a redshift that places it at a significant distance. Faint, extended halo structures are barely discernible, indicating the presence of older stars outside the main body. There is no noticeable dust lane or irregular features, and there is no apparent tidal disturbance, suggesting the galaxy is relatively undisturbed and not currently undergoing a major merger event.
