The galaxy presents as a slightly elongated, diffuse object with a relatively smooth light distribution. Its core appears bright, with the light profile gradually decreasing towards the outer regions. There is a hint of a disk-like structure, but it is not sharply defined. The color appears predominantly white with subtle hints of blue and red, possibly indicating a mix of stellar populations, with the blue suggesting some presence of younger, hotter stars. There is no clear evidence of spiral arms, distinct dust lanes, or a prominent central bar. The overall morphology suggests an intermediate stage between a pure elliptical and a spiral galaxy, possibly leaning toward a lenticular (S0) classification. Minor disturbances in the galaxy's structure may be present.
