The galaxy presents as an elliptical, cigar-shaped form. The central bulge is noticeably bright and exhibits a yellowish hue, likely indicative of an older stellar population. Fainter, bluer, extended light surrounds the central region, which may suggest regions of more recent star formation or younger stars. There is a hint of a disk like structure, though without distinct spiral arms or well-defined features. It does not appear to be undergoing any major merger events; however, some minor disturbances in its structure cannot be ruled out. Overall, the galaxy appears to be a relatively massive system, with a moderate rate of star formation.
