The galaxy presents as a single, relatively smooth object, with a slightly elliptical morphology. It appears mostly featureless upon visual inspection, lacking any obvious spiral arms or distinct substructures. A concentrated, bright central region, possibly indicating a bulge or active galactic nucleus, dominates the galaxy's luminosity profile. The color gradient transitions from a bluer hue in the outer regions, suggesting the presence of younger stellar populations, to a more yellow/red color toward the center, potentially indicative of older, redder stars and dust accumulation. The galaxy exhibits a moderate degree of roundness, not appearing highly flattened or elongated. There are no immediately apparent signs of tidal disturbances or ongoing major mergers with other galaxies, though a minor interaction cannot be entirely ruled out. Overall, the galaxy seems to be a relatively evolved system, possibly an elliptical or lenticular type, with a notable central concentration of light.
