The observed galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical galaxy. The galaxy exhibits a concentrated central bulge, with a gradual decline in luminosity outwards. The overall color appears yellowish, consistent with an older stellar population. There is very little evidence of distinct spiral arms or prominent dust lanes, further supporting the classification of an elliptical galaxy. It displays a relatively round shape. There are no major merging signatures, although there is very mild disturbance visible in the outskirts.
