The galaxy presents a somewhat elliptical morphology, with a prominent, concentrated central bulge region exhibiting a yellowish-orange hue, which suggests a population of older, redder stars. This bulge is the dominant feature, and appears relatively smooth in texture.

Fainter, more diffuse and irregular structures surround the central bulge, extending outwards. These outer regions show a mottled appearance with varying shades of red, green and blue. The varying colors indicate a mix of stellar populations; some regions may contain younger, hotter stars that contribute to the blue emission, while dust absorption may affect the redness of other regions. There are hints of faint spiral arm structures but they are ill-defined. Some minor disturbances appear present within these outer regions as well, possibly due to past or ongoing interactions with other galaxies. 

Overall, the galaxy exhibits characteristics of a disk galaxy, with a relatively substantial bulge component. The galaxy's relatively redder color profile suggests a comparatively quiescent star formation rate.
