The galaxy presents as a centrally concentrated object with a smooth overall morphology. The light distribution is largely spheroidal with a gradual decrease in intensity from the core outwards, indicating a relatively high degree of symmetry. The color profile suggests a population of older stars dominating the central regions, characterized by a yellowish-orange hue. There is a slight hint of bluer color in the outer regions, which may suggest the presence of some younger stellar populations, or potentially star forming regions, although these are not prominent. No distinct spiral arms or a prominent disk structure are discernible from the image. There does not appear to be any clear evidence of a major ongoing merger or tidal disruption. However, the overall roundness of the galaxy is not perfect and the possibility of a minor interaction with a smaller companion cannot be ruled out completely. The galaxy is generally well-defined, although the image quality does limit a detailed analysis of finer structures.
