The galaxy presents as a generally smooth, elliptical morphology, appearing largely undisturbed. There is a slight elongation, deviating from a perfectly circular shape. The color profile indicates a dominant yellowish-orange hue in the central region, potentially indicative of an older stellar population. Fainter greenish tones are present on the periphery of the galaxy, potentially signaling pockets of more recent, albeit diminished, star formation activity or a difference in chemical composition. There is no distinct spiral arm structure or prominent dust lane apparent in the image. The galaxy shows no strong signs of tidal disruption or ongoing major merger events, though subtle features could indicate past minor interactions.
