The galaxy appears to be a relatively smooth, elliptical structure. It presents with a centrally concentrated light profile, exhibiting a gradual decrease in luminosity from the core outwards. There is a slight elongation, but overall it maintains a generally round shape. No distinct spiral arm structures or significant dust lanes are observed. The color profile suggests a population of older stars, with a tendency towards redder hues. There is no apparent ongoing major merger event, nor any significant tidal disturbances visible.
