The galaxy presents a predominantly smooth morphology, appearing largely spheroidal in shape. It exhibits a concentrated central bulge with a gradual falloff in luminosity towards its outer regions. There is a slight elongation visible, suggesting it is not perfectly spherical. Hints of a faint disk-like structure may be present, but this is not distinctly defined. 

The color profile is primarily characterized by yellowish hues, indicative of an older stellar population. The galaxy lacks strong blue regions, which suggests that active, ongoing star formation is minimal. The overall light distribution is relatively uniform, further supporting the impression of a well-mixed, evolved stellar population. There do appear to be a few regions of light disturbance that indicate this galaxy may be merging with another galaxy or experiencing minor disturbances.
