The galaxy presents as a centrally concentrated object, exhibiting a largely spheroidal morphology with a smooth appearance. There's no clear presence of spiral arms or a distinct disk structure. It is highly rounded in shape, showing no significant elongation or distortion. The galaxy appears to be relatively isolated, showing no signs of ongoing major merger activity or strong tidal disturbances. There is very faint indication of minor disturbance in the overall light profile. The object appears to be of intermediate mass. The colors suggest a moderate degree of star formation activity.
