The galaxy presents as a relatively compact structure, likely a lenticular or early-type spiral, exhibiting a smooth light profile indicative of an older stellar population. The object appears nearly circular, with no strong asymmetries or tidal features discernable. Color gradients suggest a redder core, with bluer peripheries. The redder color of the core implies an abundance of older stars and a relative deficit of recent star formation. The galaxy's size on the image appears to be moderate, representing roughly 2.6 kpc. Light from the central regions dominates the overall emission. There are no apparent dust lanes, bars, or spiral arm structures visible. A small portion of the galaxy appears to show that there is some star formation present in the disk, which is the cause of the bluer peripheries. Overall, the galaxy is quiescent with respect to major star formation.