The galaxy presents a largely smooth morphology with a centrally concentrated brightness profile. It exhibits a generally elliptical shape, appearing mostly round. The galaxy's core region displays a yellowish-white hue, suggesting a population of older stars. Fainter reddish tones are detected closer to the core, potentially indicative of dust or H-alpha emission from star forming regions within the galaxy. There are no significant indications of major disturbances or merging events. A general lack of distinct spiral arm structures reinforces the smooth characteristic of the galaxy.
