The galaxy presents as a relatively smooth, elliptical-like morphology. There is a bright, centrally concentrated bulge that appears to dominate the overall light profile. The bulge exhibits a yellowish-orange hue, indicative of an older stellar population. Surrounding the bulge is a less luminous and more diffuse halo or disk component. The galaxy displays a slight elongation, with a moderate cigar shape, deviating from a perfectly circular form. There is no apparent evidence of major mergers or significant tidal disturbances. Minor disturbances are possible, but not readily discernible. The galaxy appears quiescent, with likely low star formation rates across its structure.
