The galaxy presents a distinct spiral morphology. Two tightly wound spiral arms are prominently visible, originating from a moderately sized central bulge. The arms exhibit a medium winding, wrapping noticeably around the galactic core. A weak bar structure appears to be present, subtly elongated across the central bulge, though it's not a dominant feature. The spiral arms are well-defined, hinting at ongoing star formation activity within the disk. There is no obvious indication of any major ongoing mergers or significant tidal disturbances, suggesting a relatively isolated and dynamically stable system. The overall color profile indicates a mix of stellar populations; the bulge appears somewhat redder than the arms, typical of older stars.
