The galaxy appears to be a relatively smooth and centrally concentrated system, with a general spheroidal morphology. The color profile indicates a population of older stars with a dominant reddish-yellow hue, suggesting a moderate amount of star formation. There is a slight elongation, but it is generally quite round. The faintness of any distinct spiral arms or features supports a classification towards the earlier end of the Hubble sequence. It shows no strong evidence of major mergers, however, there is a slight disturbance in the morphology. Given its estimated size of approximately 7.7 kpc across, this galaxy could be classified as a smaller sized galaxy.
