The galaxy presents a generally smooth morphology with a slightly elongated, disk-like appearance. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. Faint disk features are visible, but lack defined spiral arms. The galaxy displays a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. There is subtle evidence of minor disturbances in the outer regions, possibly indicative of a past or ongoing interaction with a smaller companion galaxy, or internal dynamics. The overall color profile indicates a relatively low level of current star formation.
