The galaxy presents as a relatively smooth, centrally concentrated light distribution, with a slightly elliptical shape. The galaxy has a bright central region, indicative of a bulge, surrounded by a fainter, more diffuse halo. There is a faint, reddish feature extending from the galaxy, suggestive of a tidal stream or possible dust lane. There are no clear spiral arm structures visible, and the overall appearance implies an early-type galaxy, perhaps an elliptical or lenticular type. The smoothness of the light distribution, combined with the lack of distinct features, suggests that the galaxy is relatively undisturbed, with no recent major merger events. The estimated mass is moderate, and the star formation rate is comparatively low. The slight elongation could indicate ongoing minor interactions or a remnant of a past merger.
