The galaxy appears as a slightly elongated, elliptical structure. The central region exhibits high surface brightness, indicative of a concentrated nucleus. The color distribution suggests an older stellar population, with a dominant yellowish-orange hue concentrated towards the center, fading into redder tones at the outer edges. There is a hint of faint, extended halo surrounding the central region, gradually diminishing in brightness. No distinct spiral arms or prominent dust lanes are discernible. Overall, the galaxy seems to be undergoing minimal star formation. There are no signs of any major mergers or tidal disturbances.
