The galaxy presents as a moderately bright, relatively compact object. Its morphology appears largely smooth, exhibiting a spheroid-like shape with hints of some internal structure. The color profile reveals a bluer core with a slight reddening towards the outer regions. This color gradient suggests the presence of younger, hotter stars concentrated in the central region, and potentially older stellar populations distributed more broadly throughout the galactic body. There is possible evidence of tidal disturbance, indicated by faint, extended features around the galaxy.
