The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge. Its overall shape is somewhat elongated, exhibiting an intermediate ellipticity, neither perfectly round nor highly flattened. The color profile suggests an older stellar population, with a dominant yellowish-orange hue. There is no obvious evidence of spiral arms or significant dust lanes. No indications of recent or ongoing major mergers or tidal disturbances are observed, although subtle irregularities in the outer regions cannot be ruled out. Given the overall smooth morphology and color, the galaxy is likely relatively quiescent in terms of star formation.
