The galaxy presents a flattened, elliptical morphology, suggestive of a disk galaxy viewed at a moderate inclination. A distinct central bulge is observed, exhibiting a yellowish-white hue, possibly indicating an older stellar population. Fainter, bluer light extends from the core, possibly tracing spiral arm structures; however, the resolution is insufficient to definitively resolve spiral arms. There may be some low level distortions of the overall shape, indicating a possible recent interaction with another galaxy, but further analysis is needed to confirm this.
