The galaxy exhibits a generally smooth morphology, with a slight elongation along one axis, suggesting a possible elliptical or lenticular classification. The central bulge is prominent and displays a yellowish hue, indicating a population of older stars. The outer regions of the galaxy appear fainter and bluer, possibly due to a small amount of ongoing star formation. There is no clear evidence of spiral arms or a well-defined disk structure. Minor distortions and irregularities in the light distribution might be present, hinting at a possible past or ongoing interaction with another galaxy. The overall color profile suggests a relatively evolved system.
