The galaxy presents as a moderately bright, elongated structure. Its color profile suggests an older stellar population, with a dominant yellowish hue concentrated towards the center, indicating a bulge. There is a hint of bluer light on the edges, perhaps suggesting some star formation, though the galaxy's dominant color suggests this galaxy is comprised of older stars. The galaxy appears relatively smooth, with a slight hint of possible disturbance, but not in any obvious major merger. The morphological classification likely leans towards elliptical or S0 type due to its shape and color.
