The galaxy presents a generally smooth morphology, with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, potentially indicative of an older stellar population. Surrounding the core, a less concentrated, bluer halo is visible, suggestive of the presence of younger stars and ongoing star formation, albeit at a relatively modest rate. The overall shape appears to be somewhat elliptical. There is no strong evidence of spiral arm structures or major disturbances within the galaxy’s structure. There is an absence of any strong signs of an active galactic nucleus or significant dust lanes obscuring the galaxy’s core. A minor asymmetry is observed, which may indicate a minor interaction, disturbance or internal process.
