The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated bulge, dominating its overall structure. The light profile appears fairly uniform, with no distinct spiral arms or bar features discernible. There is a slight elongation evident, deviating somewhat from a perfectly circular shape. The galaxy's color suggests a relatively evolved stellar population; the yellowish hue is indicative of older, redder stars within its structure. There is no clear evidence of on-going major merging events, but a very slight asymmetry hints at a possible minor interaction or internal disturbance. Star formation rate appears low, indicative of a quiescent or passively evolving system.
