The galaxy appears as a relatively smooth, elongated object. It exhibits a central bulge with a yellowish hue, suggesting a population of older stars. The overall shape leans towards a more intermediate profile rather than perfectly round or strongly elongated, with a subtle disk-like structure that is difficult to resolve due to the image resolution. There may be some disturbances suggesting a possible interaction, but no clear signs of a major merger are immediately apparent. The galaxy's morphology is most consistent with an early-type spiral galaxy or a lenticular galaxy viewed at a slight angle. 
