This galaxy presents as a relatively bright, centrally concentrated object. The core region exhibits a notably smooth and luminous profile. The surrounding galactic halo appears more diffuse, with a subtle, elongated morphology that is suggestive of a disk galaxy. There is no apparent spiral structure. The color profile reveals a yellowish hue concentrated at the core, with a gradual shift towards redder tones in the outer regions. The low degree of visible disturbance suggests the galaxy is relatively isolated and not currently undergoing a major merger event. The overall smoothness implies that star formation is low within this galaxy.
