The galaxy presents as a moderately luminous object with an elliptical morphology. It exhibits a generally smooth appearance, with a slight elongation indicating a deviation from perfect sphericity. The color profile suggests an aging stellar population, with a dominant yellowish-orange hue concentrated in the central regions. There's a subtle color gradient towards the periphery, showing hints of bluer light, possibly indicating some ongoing, albeit minimal, star formation activity in the outer regions. No distinct spiral arms or prominent dust lanes are visible. The overall structure appears relatively undisturbed, without strong evidence of recent major mergers or tidal interactions.
