The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is elliptical or lenticular, with no obvious spiral arm structure. The light distribution is dominated by a diffuse, yellowish glow. The galaxy exhibits a slight elongation, deviating somewhat from a perfectly circular shape. There is no discernible evidence of active galactic nuclei activity in the core, and no prominent dust lanes or recent merger events are visible. The overall impression is of an evolved system with an older stellar population.
