The galaxy presents as a relatively compact, disk-shaped system exhibiting an intermediate degree of ellipticity. Its central region shows a bright, concentrated core, likely indicative of a significant stellar population or active galactic nucleus. The surrounding disk appears generally smooth, with a subtle color gradient suggesting variations in stellar populations and dust content. A slight warping or irregularity is visible in the disk structure, particularly on one side, possibly indicating tidal interactions or minor mergers in its past. The color profile suggests ongoing star formation, potentially at a modest rate, with bluer regions implying younger stellar populations mixed with dust. Overall, the galaxy is likely an intermediate-mass system undergoing relatively quiescent evolution but is possibly experiencing subtle gravitational disturbances.
