The galaxy presents as a largely elliptical or lenticular structure, exhibiting a high degree of smoothness in its light distribution. It appears nearly circular in projection, with a very slight elongation. The dominant color is yellow-white, suggesting an older stellar population. A faint, diffuse extension of bluer light emanates from one side, hinting at potential ongoing star formation, possibly triggered by a minor interaction or accretion event. There is no clear evidence of spiral arms or a prominent dust lane, further supporting the classification as an early-type galaxy. Overall, the galaxy appears relatively isolated and undisturbed.
