The galaxy presents a generally smooth appearance, lacking any obvious spiral arm structures or a distinct central bar. The light is concentrated in a roughly circular, moderately compact form. Its color profile suggests a population of older stars. The central region appears slightly brighter, indicating a possible concentration of stars toward the core, but it is not a distinct or active galactic nucleus. There is no clear evidence of ongoing major merging activity or significant tidal disturbances; however, there may be minor irregularities in the outer regions of the galaxy indicative of past interactions. The galaxy's overall morphology suggests an elliptical classification, although the possibility of a tightly wound spiral galaxy cannot be ruled out based solely on this image.
