The galaxy presents as a single, relatively smooth object. Its morphology appears largely elliptical, though not perfectly circular. There is a slight elongation, suggesting a possible transition between spherical and more cigar-shaped forms. Color gradients across the galaxy are subtle, with a somewhat yellower core region fading to slightly bluer outer edges. The object displays no obvious signs of major mergers or tidal disturbances. There may be minor internal structures, potentially faint dust lanes or spiral arm remnants. The size appears moderate, neither a dwarf nor an exceptionally large galaxy. Integrated light suggests a redder spectral energy distribution, typical of galaxies with older stellar populations, though some blue light indicates ongoing star formation.
