The galaxy presents as a fairly smooth, elliptical-shaped structure. Its core exhibits a bright, concentrated luminosity, suggesting a substantial density of stars. The color profile leans towards the red end of the spectrum, indicative of an older stellar population with fewer young, blue stars. There is little evidence of distinct spiral arms or dust lanes, and no prominent star-forming regions are discernible in this image. The galaxy's overall morphology appears relatively undisturbed, with no apparent signs of a major ongoing merger or significant tidal disruption.
