The galaxy presents as an elongated, cigar-shaped structure, likely an elliptical galaxy viewed at an angle. The central region exhibits a concentration of light, appearing yellow-white, suggesting an older stellar population. The light fades gradually towards the edges of the galaxy, creating a soft, diffuse halo. There is a slight bluer tinge surrounding the bright central region, which might indicate the presence of a small population of younger stars. There is no visible evidence of distinct spiral arms or strong dust lanes, but some minor disturbances are present in the halo region. The galaxy appears relatively smooth in texture, with no clear signs of active star formation regions.
