This galaxy exhibits a somewhat elliptical morphology, appearing more cigar-shaped than round. The core region presents a yellowish-orange hue, potentially indicating an older stellar population. Moving outwards from the center, the color shifts towards a bluer tint, particularly along the edges. This suggests the presence of more recent star formation in these outer regions. There appears to be a slightly disturbed structure, indicative of a possible past or ongoing minor interaction or merger event. The galaxy appears relatively smooth, but there is some evidence of subtle features. Overall, this galaxy appears to be a moderately massive system with ongoing, though perhaps subdued, star formation.
