The galaxy exhibits a generally smooth morphology, appearing elliptical in shape with a high degree of roundness. A prominent central bulge is visible, characterized by a concentrated, yellowish light, suggesting a population of older stars. Surrounding the bulge, a less distinct disk component is observable, showing a subtle gradient in color and brightness. The overall color profile indicates a relatively low level of recent star formation, with the dominant stellar population being evolved and redder. There is a slight indication of a minor gravitational disturbance, although no major merger activity is apparent in the image. No distinct spiral arms or strong dust lanes are discernible. The galaxy appears to be relatively isolated, showing no immediate signs of interaction with neighboring galaxies.
