The galaxy presents as a dominant, relatively smooth structure with a moderate ellipticity. The central region is characterized by a strong concentration of light, appearing yellowish-orange in color, suggesting an older stellar population. This central region gradually transitions into a surrounding halo.

The outer regions of the galaxy exhibit a more complex, slightly clumpy texture, with hints of greenish-blue light. This color variation suggests the presence of younger, hotter stars possibly residing in sparse spiral structures or irregular features. The overall structure shows no clear signs of ongoing major mergers or tidal disturbances, though there may be minor asymmetry present in the outer regions. The galaxy's estimated size indicates that it is a moderately large galaxy, with the light being concentrated in the central regions. The colours suggest the presence of some ongoing star formation, but not at a very high rate.
