The galaxy presents as an elliptical morphology. There is a smooth and centralized concentration of light with a noticeable transition toward a cigar-shaped structure. The core exhibits a bright, yellowish hue that suggests an older stellar population, potentially dominated by red giant stars. Moving outwards from the core, the light diffuses gradually, with the yellow diminishing in intensity. There are faint hints of bluer regions, indicating some level of ongoing, but minimal, star formation. The lack of distinct spiral arm structure is evident, further reinforcing the assessment of this galaxy as being in a later stage of evolution, with only minor disturbances.
