The galaxy presents an overall smooth morphology, with a slightly elongated shape reminiscent of an elliptical galaxy, though some disk-like structure cannot be entirely ruled out. There is a clear central bulge that exhibits a bright, concentrated luminosity profile. Moving outward from the core, the luminosity gradually diminishes, fading into the surrounding space. The primary color is a yellow-white, suggesting a stellar population that is primarily older, with fewer young, massive stars. There's no strong evidence of prominent spiral arms or significant dust lanes. There appears to be minimal active star formation, though subtle color variations hint at the presence of some younger stars. No signs of a major ongoing merger event are observed, but the possibility of minor past interactions cannot be discounted due to the slight asymmetry in the overall shape and faint wisps of light extending outward.
