The galaxy appears as a relatively small, faint object. It exhibits a generally smooth, rounded morphology with a slightly elongated profile, though it is difficult to resolve fine details given its apparent size and distance. The color profile is fairly uniform across the galaxy, with some slight color variation. There does not seem to be a prominent disk structure. There is no evidence of any major ongoing merger events, though some small asymmetry cannot be ruled out, which could point to some degree of interaction or disturbance. Overall, the galaxy presents a somewhat unremarkable appearance, potentially indicative of an older stellar population and relatively low star formation activity.
