The galaxy presents as a moderately bright, elliptical or lenticular system at a redshift of approximately 0.12. Its central bulge region appears predominantly yellow to orange in color, suggesting an older stellar population. The surrounding halo fades smoothly outward, exhibiting a slight elongation with the major axis having an aspect ratio of approximately 3:5. There is minimal evidence of spiral arm structure or significant dust lanes. A faint greenish tint is observed near the periphery, potentially indicating the presence of some younger stars or ionized gas, although star formation appears quiescent overall. The overall morphology suggests a galaxy that is relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions.
