The galaxy presents as a somewhat elliptical, centrally concentrated structure. The light distribution appears smooth, with a high degree of symmetry relative to its major and minor axes. The core exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, bluish extensions are observed emanating from the central region, particularly along the galaxy's equatorial plane, which could indicate the presence of younger, hotter stars. The galaxy lacks any obvious signs of strong spiral arm structure or bar features. There is no visually discernible evidence of tidal tails or ongoing major mergers; however, a slight asymmetry in the outer regions could suggest minor past interactions or disturbances. Overall, the galaxy presents a relatively relaxed, evolved morphology.
