The galaxy presents as an elliptical or lenticular morphology. It exhibits a relatively smooth, centrally concentrated luminosity profile. The overall color appears yellowish-white, suggesting a population of older stars. There is a slight elongation, indicating a deviation from perfect circularity. No distinct spiral arms or significant dust lanes are visible. There appears to be little to no star formation activity occurring, or the star formation that is occurring is deeply embedded within the galaxy, and not readily apparent from the image. No signs of a major merger, tidal tails, or significant disturbances are observed. A slight asymmetry can be observed on the edges of the galaxy, indicating a minor disturbance possibly due to a smaller galaxy, but no other galaxies are observed nearby.
