The galaxy presents a generally smooth morphology with a bright central region. The shape appears more or less round. There's minimal indication of spiral arms or a distinct disk structure. The color profile reveals a subtle bluing trend toward the core, suggestive of some ongoing star formation, while the outer regions exhibit redder hues. There's no immediately obvious evidence of major mergers or significant tidal disturbances. Overall, the galaxy's appearance points towards an elliptical or lenticular classification, with the possibility of weak, centrally concentrated star formation activity.
