This galaxy presents as a largely spheroidal structure, exhibiting a high degree of smoothness with a concentrated central bulge. The galaxy appears to be relatively undisturbed, showing no significant signs of ongoing or recent major mergers. Faint color gradients suggest a possible difference in stellar populations between the core and outer regions, with the core tending towards redder hues, potentially indicating older stars or higher metallicity. The outer regions appear slightly bluer, possibly due to younger stars or ongoing star formation. Overall, the galaxy is likely an elliptical galaxy at an estimated distance corresponding to a redshift of approximately 0.24. There might be low levels of star formation occurring within the galaxy.
