The galaxy presents as a concentrated, ellipsoidal form. The core region exhibits high luminosity, with a relatively smooth, featureless appearance and a moderate degree of roundness, with a slight elongation suggestive of a weak bar or disk component viewed at an oblique angle.  There appears to be little to no evidence of distinct spiral arm structures. There is no obvious dust lane obscuration.  The galaxy's overall color is consistent with an older stellar population. There is a suggestion of minor tidal disturbance, but no significant ongoing major merger activity is apparent. Estimated to be several kiloparsecs in diameter, it is a relatively compact system. Although the color bands were not requested, given the magnitudes, the color index appears to be slightly redder than the sun. The apparent lack of notable spiral structure and overall smooth appearance suggest a possible classification as an early-type galaxy, such as an elliptical or lenticular. The lack of blue color suggests a modest or absent rate of star formation.
