This galaxy appears to be a relatively compact object exhibiting characteristics of both smooth and irregular morphologies. The central region is bright and somewhat condensed. A fainter, more diffuse envelope surrounds this central area, which has an apparent diameter of approximately 3 kiloparsecs. 

The galaxy's overall shape is somewhere between a rounded disk and a disturbed system. It is possible there is ongoing or recent tidal interaction, indicated by faint and slightly irregular features extending from the primary body of the galaxy. The overall color suggests the presence of a mix of stellar populations. There is evidence of both older, redder stars and younger, bluer stars. The blue component suggests the galaxy has not fully exhausted its star-forming material. The rate of star formation is very low. The mass is likely around 10^9 solar masses.
