The galaxy presents as a somewhat elliptical, though nearly spheroidal, system with a bright, concentrated central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. A faint, extended disk surrounds the bulge. The disk appears relatively smooth, with little evidence of distinct spiral arms. The disk's color is slightly bluer than the bulge, hinting at the presence of younger, hotter stars. The galaxy displays a mild degree of internal structure. There is little evidence of significant tidal disturbances or ongoing merger activity.
