The galaxy presents as a relatively small, moderately luminous system with an apparent reddish hue. Its morphology is primarily smooth with little to no disk-like or spiral structure discernable from the available data. The light distribution is relatively even, showing a slightly ellipsoidal shape, deviating little from a circular appearance. There is no clear evidence of any ongoing major merging events or strong tidal disturbances affecting the overall galactic structure, but there seems to be a minor asymmetry. The low redshift indicates it is a relatively nearby galaxy. The galaxy's color suggests a population of older stars and a lower ongoing rate of star formation.
