The galaxy presents as an elongated, diffuse structure with a noticeable central concentration of light. Its overall color appears to be yellowish-orange, suggesting an older stellar population. The galaxy lacks a well-defined spiral arm structure or a prominent disk. There are subtle irregularities in the galaxy's shape and luminosity distribution, possibly indicating minor gravitational interactions or internal disturbances. The edges of the galaxy are indistinct, fading gradually into the background. There may be other faint objects in close proximity. The light from this galaxy spans just under 10 arcseconds. The galaxy's overall appearance hints at it being either an elliptical or lenticular galaxy, potentially undergoing some form of interaction. A small fraction of the galaxy's light might be from younger stars or star forming regions. 