The galaxy appears as a single, somewhat smooth, and centrally concentrated object. The light profile suggests an elliptical morphology, exhibiting a rounded appearance rather than a distinct disk or spiral structure. There is a yellowish hue to the galaxy's core, possibly indicating an older stellar population. The light is fairly uniform, with little evidence of significant dust lanes or active star-forming regions. There is a very slight asymmetry in the light distribution of the halo, possibly indicative of a minor interaction, but the main body seems undisturbed. The colors suggest low star formation. 
