The galaxy presents an elliptical morphology, elongated along a discernible axis. The central region exhibits a bright, concentrated luminosity profile, suggestive of a prominent galactic nucleus. The luminosity gradually decreases outwards from the core, exhibiting a smooth transition with no apparent distinct features such as spiral arms or a bar structure. The color profile appears relatively uniform across the galaxy, with a slightly bluer hue. The outer regions are more diffuse and less well-defined than the central region. There is evidence of a minor disturbance, such as a slight asymmetry or irregularity in the outer isophotes, potentially indicating a past or ongoing minor merger event. Overall, the galaxy appears to be a relatively evolved system.