The galaxy presents a largely smooth morphology, appearing as an elliptical or lenticular system when assessed visually. There is minimal indication of spiral arm structure or prominent dust lanes. The overall color profile leans towards the red end of the spectrum, indicative of an older stellar population and a relatively low rate of current star formation. The galaxy's light profile appears concentrated with a centrally brightened region. It appears roughly round, showing minimal elongation or asymmetry which suggests a relaxed state, without current major merging activity. There is a faint extended halo of light surrounding the central region. The object appears isolated with no clear tidal features or nearby interacting companions.
