The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular type given its apparent lack of spiral arm structures. The central region exhibits a bright, yellowish-white color, indicating a population of older stars. Moving outward from the center, the galaxy gradually fades into a more diffuse halo of greenish light, suggesting the presence of a fainter, cooler stellar population, and possibly some ongoing, though subdued, star formation. The overall shape is elongated, but only moderately so, displaying a cigar-like morphology. There is no clear indication of any major mergers or significant tidal disturbances affecting the galaxy's overall structure, but there may be a hint of a minor perturbation. The galaxy appears relatively isolated, with no obvious signs of interaction with nearby companions.
