The galaxy presents a generally smooth, rounded morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. There is a subtle color gradient observed, transitioning from a bluer hue in the central region to slightly redder tones in the outskirts. This could be indicative of differing stellar populations, with potentially younger, hotter stars dominating the core and older, cooler stars populating the outer regions. There is no clearly defined disk or spiral structure discernible. The galaxy does not appear to be strongly interacting or merging with any other significant companion objects, however there may be very minor tidal disturbances or interactions with another galaxy that cannot be clearly made out in this image. Overall, the observed characteristics align with a classification consistent with a relatively evolved system.
