The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be centrally concentrated with a bright core, exhibiting a general yellow-orange hue. This color profile suggests an older stellar population dominating the light output. A slight elongation is visually discernible. There is an adjacent, smaller object visible that could be a satellite galaxy or a background object. There is no prominent disk structure or spiral arm features are detected. Overall the morphology appears relatively undisturbed.
