The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated morphology with a high degree of radial symmetry. The primary light emanates from a bright, yellowish core, indicative of an older stellar population. The core transitions smoothly into a fainter, more diffuse halo. The galaxy has an overall elongated shape, and may be approaching a cigar shaped morphology, but appears closer to round. No distinct spiral arms or dust lanes are visible. There is some evidence of minor asymmetry or a slight warp in the outer regions of the halo, potentially hinting at a past or ongoing minor merger event or tidal interaction, however this is most likely just an artifact. The lack of blue light suggests a low rate of recent star formation.
