The galaxy presents a largely elliptical morphology, exhibiting a high degree of central concentration. The light distribution is smooth, with no immediately discernible spiral arms or bar structures. The galaxy's color index suggests a relatively old stellar population, with a dominant yellowish-orange hue in the central region, fading to a more muted color in the outer regions. There is no strong evidence of ongoing major star formation activity based on the observed color profile. Faint disturbances or tidal features may be present in the immediate vicinity, warranting further investigation to determine if any minor merger events could be occuring. The object is moderately luminous, with an apparent compact size.
