The galaxy presents a predominantly smooth, elliptical morphology with an approximate effective radius of 7.6 kpc. Its light profile suggests a relatively even distribution of stellar mass. A slight elongation is observed, deviating modestly from a perfectly circular shape. The central region appears to be somewhat brighter and exhibits a yellow-reddish hue, potentially indicative of an older stellar population and/or dust obscuration. While the galaxy appears generally undisturbed, a hint of asymmetry in its outer regions might suggest a past minor interaction or internal dynamical processes. Overall, the galaxy gives the impression of a passively evolving system with a significant spheroidal component.