The galaxy presents as a smooth, elongated structure with a high degree of central concentration. Its overall shape is consistent with an elliptical or lenticular morphology viewed at an oblique angle. The core region exhibits a bright, concentrated luminosity, suggesting a significant population of older stars. The color profile is mostly homogenous, with a slight blue shift towards the edges indicating regions of more recent star formation. There are no visually apparent spiral arm structures or dust lanes. There are no obvious signs of major mergers or significant tidal disturbances.