The galaxy presents as a lenticular-like system. It exhibits a smooth, centrally concentrated bulge that is nearly homogenous in color and appears to be composed of older stellar populations. The galaxy shows an elongated, cigar-shaped morphology, indicating it is viewed at an oblique angle relative to its principal plane. Faint disc-like structure is present, with bluer hues suggesting ongoing, but relatively low, star formation. There is little evidence of spiral arms or significant morphological disturbances. The lack of substantial features suggests that the galaxy is in a relatively quiescent state, with minimal interaction or merging activity. 
