The galaxy appears to be a relatively small, spheroidal object, exhibiting a smooth light distribution. The main body of the galaxy is concentrated, with a gradual falloff in luminosity towards its outer edges. It has a generally round shape and appears largely undisturbed. A faint area of disturbance can be seen near one side of the galaxy. No prominent spiral arms or disk-like structures are evident. The galaxy is relatively isolated, without strong indications of interaction or ongoing merger activity.