The galaxy presents as a relatively smooth, centrally concentrated system. It appears largely featureless with no obvious spiral arm structures or prominent dust lanes. The light profile suggests a centrally dominant bulge or core region with a gradual decline in surface brightness towards the outer regions. The morphology is tending toward an elliptical form, although not perfectly circular.

The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region. Hints of bluer colors may be present in the outer edges, potentially indicating some degree of ongoing, or recent, star formation at the periphery. There may be some minor gravitational interaction with another galaxy, but this is not fully clear. No major disturbance or merger is directly visible, however, the galaxy is not perfectly symmetrical.
