The galaxy presents as a pair, potentially interacting. One galaxy appears as a disk, oriented nearly edge-on to our line of sight, exhibiting a pronounced central bulge and a reddish hue, suggesting a population of older stars and diminished ongoing star formation. The second galaxy appears more spheroidal and smooth in texture, with a brighter, concentrated core. It possesses a yellower color, indicative of a mix of stellar populations. There appears to be a faint bridge of material between the two galaxies, hinting at tidal interaction. No obvious spiral arm structures are discernible in the edge-on disk galaxy. Neither galaxy shows evidence of a strong central active galactic nucleus based on the available data. Overall, the system's morphology indicates a mature, likely merging galaxy pair.
