This galaxy exhibits a distinct, elongated morphology, appearing somewhat cigar-shaped. A concentrated central bulge is apparent, displaying a yellowish hue, suggesting a population of older stars. The surrounding disk component exhibits a bluer color, indicative of younger stellar populations and potential ongoing star formation. The galaxy appears relatively smooth in overall structure with some minor irregularities and a hint of asymmetry. There is no clear evidence of a major ongoing merger, although there is a slight disturbance in the structure.
