This galaxy exhibits a flattened, elongated morphology, suggesting a possible classification as an elliptical galaxy with a significant deviation from perfect sphericity. A dominant central bulge is apparent, exhibiting a yellowish-white hue, potentially indicative of an older stellar population. Fainter, bluer regions extend along the major axis. This color variation, suggests ongoing, albeit low-level, star formation within the galaxy's disk. The overall structure appears relatively undisturbed, with no obvious signs of tidal tails or major mergers. However, a minor asymmetry is observable, possibly indicating a past interaction or minor disturbance. The galaxy appears relatively smooth, with no large, well-defined spiral arms or dust lanes visible at this resolution.
