The galaxy appears as a centrally concentrated elliptical or lenticular system. It exhibits a smooth, generally featureless morphology, with a relatively high degree of central symmetry. There is no clear evidence of prominent spiral arms or a distinct bar structure. The overall color profile suggests a relatively old stellar population, with a redder color index implying a reduced rate of ongoing star formation. The observed roundness and lack of pronounced elongation are consistent with an E4-E5 classification on the Hubble sequence, although the presence of a subtle, low-contrast disk component cannot be entirely ruled out. The system may be undergoing or have recently undergone a minor merger event, given its slightly disturbed morphology. The galaxy is estimated to be quite massive, likely with a low specific star formation rate.
