The galaxy presents as a relatively smooth and centrally concentrated structure, exhibiting a morphology consistent with an elliptical galaxy. Its overall shape is elongated, though close to being round. The light profile appears to be dominated by an older stellar population, given the yellowish hue of the central region. There is evidence of a slightly bluer halo surrounding the core. No distinct spiral arm structures or significant dust lanes are apparent, suggesting a lack of ongoing major star formation. There is a small chance that the galaxy is interacting with another, however, it is most likely undisturbed.
