The galaxy appears to be a moderately luminous elliptical, exhibiting a largely spheroidal morphology. The light profile seems smooth and centrally concentrated, with no obvious spiral arm structures or a prominent disk. The central region shows a bright core that could indicate the presence of an active galactic nucleus, or perhaps a dense concentration of older stars. 

The galaxy exhibits a redder color, suggesting an older stellar population with relatively low ongoing star formation. Some slight irregularities or tidal features may be present in the outer regions, though they are not highly pronounced.
