The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears elliptical, exhibiting a near-spherical shape. There is no distinct disk or spiral arm structure visible. The galaxy displays a color gradient, with the core exhibiting a more yellowish hue, suggesting an older stellar population. The outer regions show a subtle shift towards bluer colors, indicating the presence of younger stars, although to a much lesser extent than observed in actively star-forming galaxies. No signs of ongoing or recent major mergers are apparent. There is potentially a very faint, diffuse halo surrounding the main body of the galaxy, but the signal is weak. Overall, this galaxy appears to be a relatively quiescent system, dominated by an older stellar population and lacking prominent features associated with active star formation or significant tidal interactions.
