The galaxy presents a generally elliptical morphology, exhibiting a smooth light distribution without pronounced spiral arm structures. The central bulge appears dominant and luminous, grading into a fainter, more diffuse halo. The galaxy shows a moderate degree of elongation. There is a hint of a possible tidal interaction or a faint, extended feature on one side, warranting further investigation to confirm its nature and connection to the main galactic structure. There are no distinct dust lanes visible. Overall, the galaxy is characteristic of a relatively evolved system.
