The galaxy presents as a somewhat elliptical morphology, exhibiting a distinct bulge component. The central region of the galaxy displays a concentrated luminosity with a yellow-orange hue, suggesting a population of older stars.  A fainter, bluish extension emanates from one side of the core, possibly indicative of a disk component with ongoing star formation. There is an asymmetrical distribution of light in this region, that may indicate a potential disturbance or interaction. The overall structure appears smooth and featureless, with some suggestions of disturbances. 
