The galaxy appears as a moderately bright, elliptical object. It exhibits a relatively smooth texture without distinct spiral arms or prominent dust lanes visible at this resolution. The central region is more luminous, suggesting a concentration of stars towards the galactic nucleus. The color profile suggests an older stellar population, with a dominant yellowish-red hue. The galaxy's shape is moderately elongated. There is no obvious evidence of recent major merger activity or significant tidal distortions. The galaxy likely has a considerable mass and is experiencing a low rate of star formation.
