This galaxy exhibits a roughly elliptical morphology, though with some visible irregularities in its outer structure. The core presents a bright, concentrated luminosity, suggesting a significant stellar density in the central region. Moving outwards, the intensity decreases, with a discernible halo exhibiting a mottled texture, potentially indicative of dust lanes or irregular star formation regions. Faint, diffuse extensions are observed at the periphery of the galaxy. There are hints of disturbances in the overall symmetry of the galaxy, perhaps due to a minor interaction. The color profile suggests a mixed stellar population, with a bluer hue in certain regions, indicating ongoing star formation, contrasted by potentially older, redder populations concentrated towards the center. The galaxy doesn't appear to exhibit a pronounced spiral arm structure.
