The galaxy appears to be a luminous elliptical with a smooth, concentrated central bulge. The color profile suggests an older stellar population, with a yellowish hue dominating the core region. There is a faint, diffuse disk component extending outwards along its major axis. The overall morphology is consistent with an early-type galaxy, exhibiting little evidence of spiral arm structure or active star formation. A slight asymmetry is observed in the outer regions of the disk, suggesting a possible minor interaction or disturbance.
