This galaxy exhibits a generally elliptical morphology, appearing elongated with a high degree of asymmetry. A bright, concentrated central bulge is visible, indicating a likely high stellar density in the core. The galaxy's disk component appears relatively faint and less defined, exhibiting a smooth texture. The bluer light from the disk suggests ongoing star formation, but at an apparently low rate. Faint spiral arm structures are suspected, although these may just be clumps of younger stars. There's a noticeable asymmetry in the galaxy's halo; there is a distinct red colored feature along the halo on the right side of the object, which suggests a possible tidal interaction or minor disturbance. The galaxy overall shows an intermediate redshift, suggesting it is at an intermediate cosmological distance.
