The galaxy appears as a relatively compact object. Its morphology suggests it is likely an elliptical galaxy, given its smooth appearance and lack of distinct spiral arms or a prominent disk structure. It is generally round. There is no clear sign of any major ongoing merger activity or significant tidal disturbances affecting the galaxy's overall structure. The galaxy exhibits a redder color, implying a stellar population dominated by older, cooler stars and a lower rate of ongoing star formation. The moderate size indicates that we are dealing with a galaxy of substantial mass.
