The galaxy presents as a fairly smooth, elliptical structure. Its central bulge is bright and appears yellowish-orange, suggesting an older stellar population. Moving outwards from the core, a diffuse, bluish halo is visible. There are no prominent spiral arms or dust lanes evident. The galaxy's shape appears elongated, with an axis ratio that deviates notably from a perfect circle, presenting a cigar-like shape. There is little evidence of any significant tidal disturbances or ongoing mergers. It is more likely that the galaxy has had no recent merging event occur.
