The galaxy presents a generally smooth morphology, with a slight elongation visible. The light distribution suggests a central bulge that transitions into a more diffuse disk. The core exhibits a yellowish hue, which could indicate an older stellar population. The outer regions of the galaxy are bluer, possibly indicating the presence of younger stars and ongoing star formation, though at a relatively low rate. There are no readily apparent spiral arm structures or bar features visible. Subtle distortions are observed in the galaxy's overall shape, suggesting a possible past or ongoing minor interaction or merger event.
