The galaxy presents as a relatively smooth, elliptical morphology, exhibiting a concentrated central bulge that gradually diffuses outwards into a less defined halo. The core region demonstrates a yellowish-white hue, indicative of an older stellar population, while the outer regions exhibit a slightly bluer color, hinting at some recent, albeit minimal, star formation activity. The overall shape appears elongated, with a cigar-like form. There is no clear evidence of spiral arms or significant dust lanes. There is no clear sign of ongoing merging activity or tidal disturbance, with only a hint of a disturbance to the sides.
