The galaxy presents as a centrally concentrated object with an overall smooth appearance. Its shape is approximately elliptical, leaning more toward being in between round and cigar shaped. A bright, compact core is evident, which appears almost unresolved in the image. The galaxy appears relatively isolated, displaying minimal signs of tidal disturbances or interactions with other galaxies. Faint extensions surround the core, giving the impression of a diffuse halo structure. Color gradients suggest the presence of distinct stellar populations. The inner region exhibits a bluer hue, potentially indicating ongoing or recent star formation. The outer regions show redder tones which could be related to older, evolved stellar populations. The galaxy is detected at a redshift suggesting a considerable distance. The lack of strong spiral arms or irregular features supports a classification as an elliptical or lenticular galaxy with relatively low star formation activity.
