The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing nearly round with a slight deviation from perfect circularity. The central region is bright, exhibiting a high degree of luminosity which fades outward. There are no readily apparent spiral arm structures or significant dust lanes visible within the galaxy's body. 

The color profile suggests a population of older stars. The blue light is indicative of regions with younger, hotter stars forming, but these populations seem to be overpowered. There is no evidence of major tidal disturbances, such as extended tails or bridges, suggesting it is not currently undergoing a major merger event, although the fuzzy edges suggest minor disturbances.

Based on its morphology, this galaxy may be classified as an elliptical galaxy, with ongoing, but mild, star formation.
