The galaxy presents as an intermediate morphology, exhibiting characteristics of both smooth and featured systems. The overall shape appears somewhat rounded, although there's a noticeable deviation from perfect circularity. The central bulge region shows a smooth, concentrated brightness profile, indicative of an older stellar population.

A fainter disk component is suspected, with a possible spiral arm structure; it is not clearly defined. There's a slight elongation or tidal feature extending from the primary galaxy body, suggesting a past interaction or ongoing gravitational disturbance.

Color gradients across the galaxy are apparent. The central bulge has a yellow-red hue, consistent with older stars. The possible disc may have a bluer tint. Evidence of dust lanes is inconclusive due to the image resolution, but there are dark patches that may obscure some regions.
