The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology and a concentrated central bulge. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The galaxy exhibits a slightly elongated shape, deviating from a perfect circle but not to the point of being cigar-shaped. There's no evident spiral arm structure or significant dust lane obscuration. Subtle color gradients suggest some variations in stellar populations, although they are not strongly defined. The galaxy appears relatively isolated, without any major signs of tidal disturbances or ongoing merger activity. Its overall light profile suggests a relatively old and evolved stellar population.
