The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a concentrated central bulge, with luminosity decreasing gradually towards the outer regions. The galaxy displays a smooth, diffuse appearance, lacking any prominent spiral arms or distinct dust lanes. The color profile suggests a population of older stars, exhibiting a yellowish to reddish hue, with some indication of ongoing star formation. The overall form suggests a relatively relaxed system, lacking signs of major recent merger events or significant tidal disturbances. The light distribution implies a fairly symmetrical shape, with only slight deviations from perfect ellipticity.
