The galaxy appears as a relatively compact object with a smooth overall morphology. It has a roughly elliptical shape, tending towards round, with minimal discernible features such as spiral arms or a bar. The galaxy exhibits a color gradient, appearing bluer in the central regions, likely indicating the presence of a population of younger, hotter stars undergoing active star formation. The outer regions are comparatively redder in hue. The galaxy's light distribution appears to be centrally concentrated, gradually fading outwards. There is some evidence of minor disturbances or irregular features which could indicate minor gravitational interaction with another galaxy.
