This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting minimal discernible features such as spiral arms or a prominent disk. The light distribution suggests a centrally concentrated morphology, with a gradual decrease in intensity towards the outer regions. The overall color is somewhat redder, indicative of an older stellar population and potentially lower levels of recent star formation. There is no clear evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity. The galaxy appears somewhat rounded in its overall shape, with no obvious elongation or distortion. Faint signs of minor disturbances cannot be fully ruled out due to the image resolution.
