The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It has a slightly elongated shape, presenting as cigar-shaped. The central region shows a concentration of light, possibly indicative of an older stellar population. The outer regions of the galaxy are fainter, exhibiting a more diffuse and less structured appearance. There is little evidence of spiral arms or significant dust lanes. There are no clear signs of any ongoing major merging activity or strong tidal disturbances. Based on its color, the galaxy likely has a moderate amount of star formation.
