The galaxy appears as a somewhat elongated, elliptical-like structure. The central region exhibits a concentrated, bright core with a yellowish hue, suggesting an older stellar population. Fainter, bluer light emanates from the outer regions, possibly indicative of more recent star formation activity. The galaxy does not present any obvious spiral arm structures or significant morphological disturbances. Overall, the galaxy appears relatively smooth and undisturbed, with a slightly irregular shape along its major axis.
