The galaxy presents a generally smooth appearance. The primary light distribution suggests an elliptical morphology, though with a subtle, elongated shape. There's a discernible central bulge exhibiting a yellowish hue, indicative of an older stellar population. Extending outward from the core, there's a fainter, bluer disk component. The disk suggests recent star formation, but does not show distinct spiral arms. The overall structure shows no strong evidence of tidal features or major mergers, but there may be subtle disturbances. The galaxy appears relatively isolated.
