The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge with a noticeable radial decrease in luminosity outwards. The galaxy's light distribution is generally uniform, showing no strong spiral arm features or pronounced dust lanes in this image. The morphology appears largely undisturbed, with only subtle irregularities that could indicate minor interactions or internal processes. The galaxy has a generally rounded appearance. The color profile suggests a population of older stars, as the galaxy's overall hue leans towards the redder end of the spectrum. There is no evident ongoing major star formation based on the image.
