The galaxy presents as a well-defined elliptical or lenticular structure, exhibiting a relatively smooth light distribution without prominent spiral arms or bar features. Its shape is generally round, with a slight elongation. A central bulge is visible. 

The galaxy appears to be actively forming stars, as evidenced by the presence of blue regions in the galaxy's midsection, with a higher concentration of stars and gas. The galaxy shows no indications of tidal tails or significant morphological disturbances that would suggest recent major merger activity, but there are areas of disturbance or active star formation within the galaxy. It shows some indication of past merger activity or tidal interactions.

The halo of the galaxy is not visible in the images. The light is concentrated in the center and midsection of the galaxy.
