This galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. There appears to be little evidence of distinct spiral arms or significant dust lanes. The color profile suggests an older stellar population, with a yellowish-red hue dominating the overall appearance. The morphology suggests it is not undergoing any major merging events or experiencing significant tidal disturbances. The galaxy appears to be fairly isolated and quiescent, with a dominant spheroid component and minimal disk structure.
