The galaxy presents as a relatively compact object, roughly elliptical in appearance, with a smooth texture. A bright, concentrated central bulge or core is visible, emitting strongly across multiple wavelengths, suggesting the presence of a dense stellar population or active galactic nucleus. Diffuse light extends outwards from the central region, with the general shape appearing slightly perturbed or irregular. A faint tidal tail or stream of stellar material can be observed extending away from the main body. The light in the disk appears to be disrupted, and suggests a possible interaction or past merger event. The color profile implies a mix of stellar populations, with the central bulge possibly containing older, redder stars and the outer regions displaying a bluer hue, indicative of younger, hotter stars and ongoing star formation.
