The galaxy presents as a moderately luminous, relatively smooth, and centrally concentrated object. Its morphology appears to be primarily spheroidal, exhibiting a lack of prominent spiral arms or a well-defined disk. The core region displays a bright, almost stellar-like nucleus, surrounded by a diffuse, yellowish halo. The overall color profile suggests a population of older stars, with limited evidence of ongoing, widespread star formation. A slight asymmetry can be observed in the outer isophotes, indicating potential minor gravitational interactions or past mergers. There are no obvious dust lanes or features indicative of recent major disturbances. The galaxy appears somewhat rounded, deviating only subtly from a perfectly circular shape.
