The galaxy exhibits a generally smooth morphology, though some irregular features are apparent upon closer inspection. The light profile is centrally concentrated, but not perfectly spherical. It appears moderately elliptical, with an intermediate degree of roundness. There is a noticeable asymmetry in the galaxy's structure, potentially indicative of a mild gravitational interaction. Furthermore, there's a bright area suggesting there's likely a region of star formation within the galaxy. Based on the color profile, the stellar population is comprised of both younger, bluer stars and older, redder stars. The overall color suggests an intermediate age for the galaxy.
