The galaxy presents as a somewhat diffuse object with a slightly elongated morphology. A central, bright region is apparent, possibly indicative of a galactic bulge or active galactic nucleus. Emanating from this central region is a fainter, surrounding structure that suggests a disk-like component, however it is not clearly defined. Subtle irregularities are noted in the outer regions of the galaxy. The color distribution suggests variations in stellar populations or dust content throughout the galaxy's structure. Faint extensions or tidal features, although not entirely distinct, hint at potential past or ongoing interactions with other galaxies, though based on the image these do not appear to be major disturbances.
