The galaxy presents as a relatively smooth, lenticular object with a central bulge and a fainter, more diffuse disk component. The overall shape is elongated, exhibiting a cigar-like morphology. There is a slight color gradient visible, with the central region appearing more red-toned, possibly indicating an older stellar population. The outer regions appear slightly bluer, suggesting some recent star formation, although the general smoothness implies a relatively low star formation rate. There is no clear evidence of spiral arms or any major disturbances indicating a recent merger event, but minor irregularities in the outer disk regions could point to past interactions. The galaxy's light profile is fairly concentrated, consistent with an object dominated by an evolved stellar population.
