This galaxy presents a primarily smooth and rounded morphology, with a concentrated central bulge. The overall color profile suggests an older stellar population, with light tending toward the redder end of the spectrum. There's a slight indication of a disk structure, but this is not sharply defined. There is a possibility of minor interaction or disturbance within the galactic structure. The galaxy does not exhibit a strong spiral arm structure or significant dust lane obscuration based on this imaging. The galaxy appears relatively isolated, not showing signs of being involved in any major merger events.
