The galaxy presents a predominantly smooth morphology, with the light appearing concentrated and centrally located. The object exhibits an elliptical shape. The color profile suggests a higher concentration of older stellar populations, visible as a yellowish hue. There seems to be little indication of spiral arm structures or significant dust lanes. This galaxy appears to be a part of a pair or an interacting system, with another galaxy in close proximity. There seems to be some disruption in the object, potentially because of the interaction, but the effect is minor.
