The galaxy presents as a centrally concentrated object with a predominantly smooth morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. A fainter, bluish extension is apparent on one side of the core, potentially indicative of ongoing or recent star formation within a disrupted region. There seems to be evidence of potential disturbances in the galaxy's structure. The overall shape is somewhat round. The faintness of the galaxy suggests it's a fair distance from our own.
