This galaxy presents as a relatively smooth, disk-like structure, observed at an oblique angle. It appears elongated, with a cigar-shaped morphology. The central region exhibits a concentration of older stellar populations, indicated by the yellowish-orange hue, which suggests diminished star formation activity in this area. Faint bluish tones at the periphery imply the presence of younger, hotter stars, potentially marking regions of ongoing or recent star formation. There is no visible evidence of a major merger, but there are some irregularities, such as a slight knot or disturbance on the edge, suggesting a possible minor interaction or internal structure. The overall form points towards it being a massive galaxy with a substantial stellar mass, though exhibiting a moderate rate of star formation relative to its mass.
