The galaxy appears as a centrally concentrated luminous object, with a relatively smooth and diffuse morphology. It displays an elliptical or lenticular shape, with no discernible spiral arms or bar structure. A gradual decrease in luminosity is observed from the central region outwards. The galaxy exhibits a color gradient; the central region presents a yellowish-white hue suggesting an older stellar population, while the outer regions show a faint bluish tint, possibly indicating the presence of younger, hotter stars, though this is less prominent. There are suggestions of possible disturbances in the galaxy's structure, with some asymmetry or tidal features perhaps present, though subtle. These potential disturbances could be indicative of past or ongoing interactions with other galaxies. Overall, the galaxy presents as a massive system with characteristics of relatively low star formation.
