The galaxy presents as a fairly smooth, elliptical-like structure with a bright, concentrated central bulge. The light distribution suggests an older stellar population, particularly concentrated within the core. There is a hint of a disc, but overall it looks undisturbed. The galaxy exhibits a reddish hue, indicating that its stellar population has most likely ceased forming stars and consists mainly of older, redder stars. The overall morphology is relatively simple, and there is no clear evidence of any major interactions or recent merger events. It appears to be a fairly isolated, evolved galaxy.
