The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a significant concentration of stars. The overall color appears yellowish, consistent with an older stellar population and a relatively low rate of ongoing star formation. A slight elongation is visible, though the object is primarily round. There's no clear evidence of spiral arms or significant dust lanes. There are no signs of significant tidal disturbances or ongoing major merger activity, although there may be some minor disturbance, or an ongoing minor merger. The galaxy exhibits a red shift, suggesting that it is relatively distant.
