The galaxy presents a notable cigar-shaped morphology, appearing elongated with a high aspect ratio. Its color profile suggests a mix of stellar populations, with a slightly bluer central region and a redder periphery. This color gradient could indicate ongoing star formation in the galactic core, gradually diminishing towards the outer regions where older, redder stars dominate. There are indications of minor disturbances in the galaxy's structure, but they are subtle. The galaxy does not show significant signs of tidal interactions or major mergers. The overall appearance points towards a relatively isolated system with a moderate level of internal activity.
