The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests a classification leaning towards elliptical or lenticular. The light profile appears diffuse, with a gradual decline in intensity from the core outwards. The galaxy exhibits a slight elongation, deviating marginally from a perfectly circular shape. There's minimal evidence of spiral arm structures or significant dust lanes within the visible spectrum. The color profile is generally yellowish-white, indicative of a population of older stars and a lack of ongoing, vigorous star formation. Subtle hints of a surrounding halo can be perceived, fading into the background. There are no obvious signs of major mergers or tidal disturbances, although minor irregularities cannot be ruled out based on this image alone. The structure is generally undisturbed, with no obvious active galactic nucleus. 
