The galaxy presents as a slightly elongated, smooth object. The color profile suggests a relatively evolved stellar population, displaying a yellow-orange hue in the central region. There is evidence of some bluer light in the galaxy, which may indicate ongoing, though subdued, star formation. The galaxy lacks a distinct disk structure, appearing more spheroidal. There is no immediately obvious presence of strong spiral arms or a central bar. The galaxy appears relatively isolated, showing no obvious signs of a major ongoing merger or significant tidal interactions with nearby companions. There might be a faint disturbance or irregularity in its overall morphology.
