The galaxy presents a predominantly smooth morphology, with a central bulge region that appears more luminous and concentrated. The overall shape is somewhat elliptical but exhibits noticeable irregularities, suggesting potential disturbances or interactions. While the majority of the galaxy's light is concentrated in the central region, there's a discernible disk component extending outward. The color profile indicates a mix of stellar populations, with the core appearing bluer than the outer regions. There is possible evidence of a recent or ongoing merger event, as the outer regions appear warped and asymmetric. There may be active or recent star formation occurring, however this is mostly contained to the central region of the galaxy.
