This galaxy presents a morphology consistent with an early-type system, likely an elliptical or lenticular galaxy. The light profile exhibits a centrally concentrated brightness, gradually diminishing outwards with a smooth appearance. The galaxy's overall shape is close to round, showing only a slight deviation towards an elongated form.

There is some suggestion of subtle, disturbed features, perhaps indicating minor gravitational interaction with a companion or the remnants of a past merger event. These are seen as faint asymmetries or irregularities in the outer regions. It displays a color gradient, with the core appearing yellower compared to the bluer outer regions. This color difference could indicate a higher concentration of older stellar populations in the core and relatively ongoing star formation.
