The galaxy presents as a relatively compact object with a smooth, somewhat elliptical morphology. Its color profile suggests a population of older stars, exhibiting a yellowish hue, concentrated towards the center. There is subtle evidence of a disk-like structure or faint spiral arms, but it is not the dominant feature. Overall, the galaxy's structure is fairly regular, with a low probability of major mergers or significant disturbances. A minor disturbance cannot be ruled out. Star formation appears present, however, based on the light profile, it does not appear to be the dominant process at this time. The galaxy displays an intermediate roundness, not entirely spherical nor highly elongated.
