The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated, bright yellowish-white luminosity, suggesting an older stellar population with minimal ongoing star formation. The light gradually diminishes outwards, transitioning to a redder hue in the outskirts of the galaxy's halo. Faint spiral arm structures may be present but are not readily discernible, possibly indicating either a very tightly wound spiral or a galaxy undergoing morphological transformation, with indications of a minor disturbance that is non-merger related. The galaxy appears well-defined, with a generally round shape, although a slight ellipticity can be observed.
