The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology with a slight elongation. It possesses a prominent bulge, characterized by a yellowish-orange hue, indicative of an older stellar population. The overall shape is somewhat elliptical, leaning towards a cigar-like appearance, with the major axis significantly larger than the minor axis. There is no clear evidence of spiral arm structures or significant dust lanes. Based on the color and smooth profile, the galaxy appears to be relatively evolved with a low rate of star formation activity. There are no signs of any major mergers or significant tidal disturbances affecting this galaxy. The galaxy seems to be a relatively isolated system.
