The galaxy presents as a diffuse, moderately resolved object. It appears to have a predominantly smooth morphology, with no obvious spiral arm structures or a well-defined disk. The light distribution suggests a centrally concentrated brightness profile, with a gradual decrease in luminosity towards the outer regions. There is a slight elongation, but the galaxy is largely round in appearance. The galaxy exhibits a subtle color gradient, with a bluer central region potentially indicating ongoing star formation and redder, older stellar populations dominating the outer edges. There's no strong evidence of active galactic nuclei activity or recent major mergers. Overall, the galaxy seems to be a relatively quiescent system, likely an elliptical or lenticular galaxy.