The galaxy presents as a relatively smooth, elliptical-like structure with a slight elongation. Its color profile suggests a population of older stars, exhibiting a yellowish hue. There is a subtle suggestion of a central bulge, but the light is fairly evenly distributed across the galaxy's body. No distinct spiral arms or active star-forming regions are readily apparent. There is a possibility of minor gravitational interaction with a neighboring object. The overall morphology indicates an evolved system, potentially with suppressed star formation.
