The galaxy appears to be a relatively smooth, elongated structure. The central bulge exhibits a concentrated, bright, yellowish-white hue, suggesting a high density of older stellar populations. Progressing outward from the core, the galaxy fades into a less defined, somewhat elongated halo. There is no apparent spiral arm structure or prominent dust lane obscuration visible in the image. The smooth morphology implies that this is likely an elliptical or lenticular galaxy, potentially undergoing passive evolution with a low star formation rate. A slight asymmetry is present, perhaps indicating a past minor merger event, but it appears mostly undisturbed.
