The galaxy presents as a single, centrally concentrated object, exhibiting a somewhat elliptical morphology. The light distribution appears relatively smooth, with a dominant central bulge that transitions into a more diffuse outer region. 

The color profile suggests a degree of spatial variation in the stellar populations. The central region is characterized by a yellow-white hue, potentially indicative of older, evolved stars. A redder component is visible on one side of the core, potentially indicating a region of active star formation or a population of dust-obscured red giant stars. No distinct spiral arms or prominent dust lanes are visible. A blueish halo may be present.
