The galaxy appears to be a relatively smooth, elliptical galaxy at a redshift of approximately 0.24. It presents a centrally concentrated luminosity profile with a dominant, spheroidal component. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a color gradient, with a yellowish-white core becoming slightly bluer towards the outer regions. This may indicate older stellar populations dominating the core, with relatively more recent, though still subdued, star formation occurring in the periphery. There might be signs of minor disturbances. Overall, this galaxy likely exhibits characteristics of a well-formed galaxy.
