The galaxy presents as a concentrated central bulge with a moderate distribution of light. It appears relatively smooth in overall morphology, with a slight elongation to its shape, leaning toward a disk-like appearance. No prominent spiral arm structures are observed, and the disk lacks a defined structure. There is a subtle colour gradient, with a slight reddening towards the central region which may indicate an older stellar population compared to the outer regions. There is some evidence of minor disturbances in the outer regions, which may be due to a weak interaction with a nearby object. The galaxy appears to be a relatively massive system with a moderate rate of star formation.
