The galaxy presents as a moderately bright, elliptical-like object with a smooth overall appearance. Its color profile suggests a relatively older stellar population, with a yellowish-orange hue dominating the central region. There is no discernible spiral arm structure or prominent dust lanes visible in this image. The galaxy appears mostly uniform. The object exhibits a degree of elongation. There is no strong evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's morphology, although minor disturbances cannot be ruled out.