The galaxy presents as an elliptical morphology, exhibiting a generally smooth and diffuse light distribution. It shows a moderate ellipticity, appearing nearly round, with a slight elongation along one axis. The galaxy possesses a bright central region that fades gradually outward without any distinct spiral arm structures or prominent dust lanes visible. The color profile suggests a redder stellar population, with a yellowish hue dominating the overall appearance, which may indicate a population of older stars and a relatively low rate of on-going star formation. There are no obvious signs of major disturbances indicative of recent mergers, although some faint irregularities in the outer regions can’t be entirely ruled out at this resolution. Overall, the galaxy appears to be a relatively evolved system, possibly in the process of transitioning towards a more quiescent phase of its evolution.
