The galaxy appears as a somewhat smooth, disc-shaped object with a slight central bulge. The central region exhibits a brighter, more concentrated luminosity, suggesting a higher density of stars and possibly an active galactic nucleus, though no distinct jet or emission is visible in this image. The disk component displays a subtle spiral structure, hinted at by faint, elongated features extending outwards from the central region. The galaxy exhibits a blueish hue, potentially indicating ongoing star formation within the disk. The overall shape is moderately elliptical, with a ratio of major to minor axis indicating a possible inclination relative to our line of sight. There may be evidence of minor tidal disturbances on one side, potentially indicating a past or ongoing interaction with a smaller companion galaxy or gravitational interactions. The galaxy's color suggests it's relatively active, and the mass indicates it's likely a spiral galaxy.
