The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated, bright core, suggestive of an older stellar population, emitting light across the yellow and green spectrum. The outer regions of the galaxy display a fainter, less structured appearance. There is evidence of a subtle disk or perhaps faint spiral features within the outer halo, but these are not clearly defined. The galaxy appears to be relatively isolated, displaying no major signs of ongoing merger activity or tidal disruption.
