The galaxy presents as a roughly elliptical, disk-shaped structure. It appears mostly smooth in overall texture, with a high degree of central concentration. The light distribution suggests it is more elongated than circular. Its color exhibits a strong central bulge of a yellowish-white hue, indicating a relatively older stellar population. Fainter, bluer light extends from the center of the bulge out towards the edges of the disk. This suggests that the galaxy's outer regions likely contain younger stars than are found at the center. There is no visible evidence of a major ongoing merger, although there might be slight morphological irregularities to the extent that minor gravitational disturbance cannot be ruled out. Overall, this appears to be a relatively massive galaxy with a relatively low rate of star formation.
