The galaxy appears as a smooth, elliptical-like structure, elongated in shape. A central, concentrated bulge of what appears to be older stars gives off a yellowish hue. Fainter, bluer light surrounds the central region, suggesting the presence of some younger stellar populations. There appears to be little to no defined spiral arm structure or dust lanes visible. The overall morphology suggests a lack of significant recent merger activity or major disturbances, though there is potentially a slight asymmetry visible in the outer regions, which may hint at a minor past interaction. The galaxy's apparent smoothness indicates that star formation is distributed rather evenly throughout, as no clear knots of active star-forming regions are visible.
