The galaxy appears as an elliptical or lenticular system, exhibiting a smooth, diffuse morphology with no prominent spiral arms or distinct features. Its overall shape is somewhat elongated. The core region presents a concentrated luminosity with a yellowish hue, suggesting a population of older stars. Moving outward from the center, the light gradually fades into the surrounding space, showing a faint blueish tint. The absence of clear dust lanes or star-forming regions points to a relatively quiescent state with likely suppressed recent star formation. There is no apparent evidence of major mergers or tidal disturbances.
