The galaxy exhibits a predominantly elliptical morphology, appearing elongated in shape. Its central region presents a bright, concentrated luminosity, suggesting a significant stellar density within the galactic nucleus. The overall color profile leans toward warmer tones, with a pronounced reddish-orange hue, indicating a population of older stars and relatively low ongoing star formation. A smooth texture is observed across the galaxy's surface, implying a well-mixed stellar population and the absence of prominent spiral arms or other distinct features. There is no indication of any major merger events or significant tidal disturbances in its immediate vicinity. Overall, the galaxy appears as a mature, relatively quiescent system.
