This galaxy appears to be an elliptical or lenticular type, exhibiting a predominantly smooth morphology. It is observed to have a generally rounded shape. The light distribution is concentrated towards the center, exhibiting a bright nucleus which fades out towards the edges. There is some evidence of minor interaction or disturbance nearby, showing a clump of light that could be a smaller satellite galaxy or tidal debris. The colors suggest an older stellar population, with a reddish-yellow hue dominating the image. This is consistent with a relatively low star formation rate and a high mass.
