The galaxy presents as a relatively smooth, elliptical-like structure. Its light is concentrated in the center, exhibiting a significant central bulge. The color is predominantly bluish, suggesting the presence of younger, hotter stars and possible ongoing star formation, though the smoothness of the galaxy indicates it is not actively star-forming. There is little evidence of spiral arms or a distinct disk structure. The morphology appears largely undisturbed, without major signs of merging activity or tidal features, although a very slight asymmetry is visible in the outer regions. This is likely a spheroidal galaxy, potentially an elliptical or lenticular type.
