The galaxy presents a somewhat irregular, elongated morphology, exhibiting characteristics of both spiral and elliptical galaxies. The central bulge appears prominent and spheroidal, displaying a yellowish-orange hue, suggesting a population of older stars. Fainter, bluer regions extend outwards from the central bulge, potentially indicating the presence of spiral arms and ongoing star formation. There is a slight hint of asymmetry in the disk component, possibly indicative of past or ongoing interactions, or internal disturbances. Overall, the galaxy demonstrates a complex structure, suggesting it has undergone a rich evolutionary history.
