The galaxy presents a relatively smooth morphology, with an overall elliptical shape. The central region exhibits a bright, concentrated core, potentially indicative of an active galactic nucleus or a dense stellar population. A faint, extended halo surrounds the core, gradually fading into the background sky. Subtle color variations are observable within the galaxy. The central core appears slightly bluer compared to the outer regions, suggesting the presence of younger, hotter stars or ongoing star formation. There is some slight evidence of a disk structure with faint arms. There might be a minor tidal disturbance or interaction with a smaller companion galaxy, as evidenced by a slight asymmetry in the halo.
