The galaxy presents as a slightly elongated, moderately inclined spiral or lenticular galaxy, exhibiting a generally smooth light distribution. It's orientation is approximately north-south with its center being slightly less bright than the outer parts. The object's relatively featureless appearance suggests it might be a more evolved system. Indications of minor disturbances may be visible in the form of subtle asymmetries in the galaxy's outer regions. The redder color profile observed suggests a population dominated by older stars and perhaps a lower rate of on-going star formation. The overall morphology hints at a galaxy undergoing, or having recently undergone, some form of interaction or merger event.
