The galaxy appears as a moderately bright, centrally concentrated object with an overall smooth morphology. It exhibits a slightly elongated shape, deviating from a perfectly circular form. There is a subtle hint of a disk-like structure, although it is not prominently defined. No spiral arms or bar features are readily apparent. The color profile suggests a relatively evolved stellar population, with a predominantly yellowish-white hue. There is no strong evidence of ongoing major merger activity, though a minor disturbance cannot be entirely ruled out given the slight asymmetry in its form. The object appears relatively isolated, without any close companions or signs of tidal interactions with other galaxies in the immediate vicinity.
