The galaxy presents as a moderately bright, elliptical structure, exhibiting a relatively smooth morphology without prominent spiral arms or a well-defined disk. The color profile is dominated by yellow and red hues, suggesting a population of older, cooler stars with ongoing star formation. The central region appears bright and concentrated. There's a subtle color gradient from the center outwards, with slightly bluer tones towards the edges indicating some presence of younger stars in the outskirts. There is no obvious evidence of a major merger event or significant tidal disruption, however there may be subtle minor disturbances in the outer regions.
