The galaxy appears as a relatively smooth, concentrated object with a somewhat elliptical morphology. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue, particularly in the central region. A subtle, faint bluish tint is observed at the outer edges, possibly indicating a small population of younger, bluer stars or some ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible. The galaxy seems to be relatively isolated, showing no strong signs of tidal disruption or interaction with other galaxies in its immediate vicinity. There's a hint of a slightly elongated shape, but overall, it's a fairly regular, centrally concentrated system.
