The galaxy presents as a single, relatively smooth, luminous object. Its morphology appears generally elliptical, exhibiting a high degree of circular symmetry. The core is highly concentrated with a bright, intense luminosity, which seems to fade gradually outward. The color profile suggests a population of older stars, with a slight reddish hue perceptible in the outer regions. There is no clear evidence of spiral arms, dust lanes, or significant star-forming regions discernible in the image. No signs of tidal interactions or ongoing mergers are visually apparent. The galaxy appears to be a relatively isolated system.
