The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards the outer regions. There is no obvious spiral structure or distinct features such as prominent dust lanes or star-forming regions visible in this image. The overall color is somewhat redder, suggesting an older stellar population and a lower rate of current star formation. The galaxy appears fairly isolated, without any strong evidence of recent or ongoing mergers or tidal interactions. There might be a hint of minor disturbance in its shape, but further analysis would be needed to confirm this. The galaxy shows a generally rounded morphology.
