The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, without prominent spiral arms or a distinct disk structure. The light distribution suggests a concentration towards the center, with a gradual decrease in luminosity moving outwards. The core region displays a yellowish hue, transitioning to reddish and bluish tones in the outer regions. Based on the galaxy's overall appearance, there is no evidence of a major ongoing merger or significant tidal disturbances. However, subtle asymmetries in the outer isophotes might indicate minor past interactions. The high degree of central concentration and smooth light profile suggest the galaxy is a relatively evolved system. Star formation activity appears to be relatively low. The galaxy is likely dominated by an older stellar population. The morphology is overall consistent with a spheroidal system, likely an elliptical galaxy or a lenticular galaxy seen close to face-on.
