The galaxy presents as a single, relatively smooth object with a generally elliptical morphology. There is a slight elongation visible, suggesting it is not perfectly spherical, but rather somewhat cigar-shaped. The radial color profile suggests a concentration of light in the central region, with a gradient towards fainter, redder hues in the outer regions. There may be a disk component, however the galaxy's smooth nature suggests it's mostly spheroidal.

Visually, there are no signs of major ongoing mergers or significant disturbances to its overall structure, although a possible minor asymmetry could be interpreted as a previous interaction. The relative smoothness and color profile are indicative of an evolved system, and the lack of prominent blue regions suggests a low current rate of star formation. 
