The galaxy presents as a relatively smooth, rounded structure. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population. Fainter, diffuse light extends outwards from the core, forming a roughly circular halo. There is some evidence of subtle color variations within the outer regions, perhaps indicating some ongoing, though relatively low, levels of star formation. No distinct spiral arms or bar structures are visible. The galaxy exhibits no signs of tidal disturbances or interactions with other galaxies.
