The galaxy presents as a somewhat elongated structure, suggesting a possible elliptical morphology, though some disk-like characteristics cannot be ruled out. The core of the galaxy appears as a bright, concentrated region exhibiting a yellow-orange hue, indicative of an older stellar population. The outer regions show a bluer tinge, hinting at the presence of younger stars and potential star formation, albeit not dominant. There is a secondary, less defined object seemingly interacting with the main galaxy on the left side of the image. It displays a similar yellow-orange color to the main galaxy's core. The main galaxy appears relatively smooth, but there are subtle indications of tidal features or minor disturbances. The overall color profile suggests a mix of stellar populations, with a likely dominance of older stars in the central bulge and some ongoing or recent star formation in the outer regions.
