This galaxy appears to be an elliptical type, exhibiting a smooth, diffuse morphology without readily apparent spiral arm structures. The light distribution suggests a centrally concentrated bulge that gradually fades towards the outer regions. The galaxy presents a slightly elongated shape. The color profile is consistent with an older stellar population, as the light is skewed towards redder wavelengths in the outskirts, with a somewhat bluer core, potentially indicating some ongoing, albeit relatively low, levels of star formation. There is a minor visible perturbation located to the left of the center.
