The galaxy presents as a generally elliptical object, exhibiting a smooth, centrally concentrated morphology. The core is a bright, yellowish-white, suggesting a significant population of older stars. Moving outwards from the core, the color subtly shifts to a more reddish-orange hue, perhaps indicative of dust or a change in the stellar population. There is little evidence of spiral arm structure, indicating a later-type galaxy, possibly an elliptical or lenticular galaxy. Overall, there appear to be no signs of any major merging events or significant tidal disturbances. The roundness is in between a perfect circle and cigar shape.
