The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. It exhibits a diffuse halo extending outwards from a brighter central region. A subtle color gradient is visible, with the central region appearing slightly more yellow-red compared to the more blue-green outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. There is a small chance it is experiencing minor disturbance, however there is no obvious signs of merging activity. Overall, it seems like a rather ordinary galaxy, fairly compact, and with little indication of strong star formation.
