The galaxy presents an overall elliptical morphology, appearing mostly smooth in texture. There is a slight elongation observed, with the major axis oriented approximately horizontally in the image. The central region exhibits a higher surface brightness, suggesting a concentrated stellar population or active galactic nucleus. Faint extensions are visible emanating from the core, with hints of diffuse light that may indicate a stellar halo or tidal features. There is a very slight blue tinge to the overall structure which may be due to star formation, but very little of the characteristic features of active star forming galaxies are readily apparent. No spiral arms are discernible. There's no visible interaction with companion galaxies, even though there is the possibility of a minor disturbance going on. Based on the available data, it is likely a relatively massive galaxy with relatively low star formation activity.
