The galaxy presents an elliptical morphology, appearing as a largely featureless, smooth distribution of light. The light is concentrated towards the center, forming a bright, well-defined nucleus. The galaxy exhibits a radial gradient in luminosity, with the central region significantly brighter than the outer regions. The overall color appears to be yellowish, suggesting an older stellar population. There is no clear evidence of spiral arms or dust lanes. The shape is somewhat elongated, but it is closer to round. Any signs of tidal disturbances, strong star formation regions, or significant morphological complexities are not visible at this resolution. The galaxy likely has a high mass and low star formation rate.
