The galaxy presents as a relatively compact, elliptical system, approximately 5.8 kpc in radius. Its overall color is yellowish-white, suggestive of an older stellar population. It shows a smooth morphology with no clear spiral arm structures. The galaxy is not perfectly round, but rather, has an intermediate shape. There appears to be a minor disturbance on one side of the galaxy, potentially indicating a past or ongoing interaction or merger event, supported by the slight irregularity in its shape. Additionally, the brightness of the galaxy suggests an average star formation rate.
