The galaxy presents as a single, moderately bright object with an elliptical morphology. The color gradient suggests a centrally concentrated population of older stars, exhibiting a yellowish-orange hue in the core that gradually transitions to a cooler, greenish-blue in the outer regions. The overall appearance is smooth with no obvious spiral arm structure or significant dust lanes visible, indicating a relatively evolved system. Faint hints of a very slight disk may be present at the periphery. There is no indication of active galactic nucleus activity or significant recent merger events.
