The galaxy presents as an elliptical or lenticular structure, with a smooth, diffuse light distribution. A distinct central bulge is observed, exhibiting a yellowish hue. The outer regions of the galaxy appear less concentrated, fading into the background sky. There is no apparent spiral arm structure. The overall morphology suggests a relatively evolved system, potentially lacking significant ongoing star formation. Faint disturbances are possibly seen in the outer regions, but with the limited detail of the image, the degree of interaction is difficult to determine. The elongated shape indicates the galaxy may be in-between round and cigar-shaped.
