The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in structure, lacking prominent spiral arms or other distinct features typically associated with disk galaxies. There's a concentrated central bulge, which graduates into a more diffuse halo. The color profile suggests a relatively evolved stellar population, with a higher concentration of older, redder stars. No signs of active galactic nuclei or major ongoing star formation are readily apparent from the image. There is no obvious evidence of tidal disturbances or merging events, suggesting it is a relatively isolated system that is undisturbed and not in the process of a merger.
