The galaxy presents as a moderately bright, relatively compact object. Its morphology appears predominantly smooth, lacking the distinct spiral arms or bar structures characteristic of some galaxies. There is a slight elongation, making it appear somewhat oval rather than perfectly spherical. The color profile suggests the presence of a relatively old stellar population. A faint and subtle disk is apparent, but only barely so. There are no signs of recent or ongoing major merger events. Any disturbances are minor. 
