The galaxy appears to be a lenticular or elliptical galaxy, exhibiting a generally smooth and rounded morphology. A bright central bulge dominates the structure, suggesting a high concentration of stars towards the galactic nucleus. There is a slight elongation or flattening of the galaxy shape, hinting it may be more akin to a lens shape than a pure sphere. No distinct spiral arms or bar structures are visible. The overall color is yellowish-white, implying a relatively old stellar population with a low rate of ongoing star formation. Hints of bluer light are extremely subtle, and limited to the galactic disc, suggesting that minimal star formation is occurring here. No evidence of a major merger or tidal disruption is observed, though a minor disturbance is possible. 
