The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The light distribution suggests a structure approaching circular symmetry.  There is minimal discernible substructure within the galaxy's body. The galaxy appears to have a yellowish hue, with a relatively homogenous color distribution. There are no obvious spiral arms, bar features, or dust lanes visible. Based on the faint distortions that are present, there may be a possible minor interaction or disturbance.
