The galaxy presents as a centrally concentrated object with a smooth light distribution. Its overall shape appears intermediate between elliptical and disk-like. A faint, diffuse halo surrounds the central region, extending further along the horizontal axis than the vertical axis. There is possible evidence of minor tidal disturbance or asymmetry in the outer regions on the left side, with a faint extension visible. The galaxy exhibits a bluish-white core, suggestive of ongoing star formation. The outer regions show more yellowish hues which may be indicative of an older stellar population. 
