The galaxy presents as a centrally concentrated object with a smooth, diffuse light profile. Its morphology appears to be largely elliptical or lenticular, with a high degree of symmetry. The core region is brighter and exhibits a yellowish hue, suggestive of an older stellar population. Moving outward, the color appears to shift towards blue, possibly indicating some presence of younger stars. The overall shape is somewhat elongated. There is no strong evidence of spiral arm structure or a prominent disk, although a subtle flattening is observed. No significant signs of tidal disturbances, major mergers, or active galactic nuclei are readily apparent from the image. The galaxy appears relatively isolated and undisturbed.
