The galaxy presents as a complex system, potentially exhibiting morphological disturbance indicative of an interaction or merger. The system appears to consist of at least two distinct components. One component has a centrally concentrated luminosity profile, suggestive of an elliptical or spheroidal morphology. The second component displays a more disk-like structure, with a faint, extended halo surrounding a bright nucleus. The disk appears somewhat distorted, possibly due to gravitational interaction. The color of the galaxy suggests an older stellar population, particularly within the central bulge and the spheroid-like component. Low star formation activity is likely taking place. The overall shape is neither completely smooth nor highly irregular, showing properties of both smooth elliptical galaxies and those with disk and/or irregular structures. A tidal tail or bridge of material connecting the two components is not readily apparent in this image, though some distortion suggests a previous or ongoing interaction.
