The galaxy appears to be an elliptical type, characterized by a smooth and relatively featureless structure. It exhibits an elongated shape, leaning towards an "in between" roundness classification. The galaxy's core appears somewhat brighter and more concentrated than its outer regions. The light distribution appears relatively even, with no prominent spiral arms or dust lanes visible. There is an indication of an interacting galaxy in the form of a close proximity with a possible tidal distortion. The colour index suggests a population of older stars, leaning more towards the redder end of the spectrum.
