The galaxy presents as a single, relatively smooth object with a centrally concentrated light profile. It appears elliptical in shape with an axis ratio of roughly 0.8, suggesting a moderate degree of flattening. The galaxy lacks any obvious spiral arm structure or prominent dust lanes. There may be minor disturbances, but the galaxy does not show evidence of a major merger event. The color appears relatively uniform across the galaxy, indicative of an older stellar population, with no distinct blue regions suggesting recent star formation.
