The galaxy presents as a centrally concentrated object with a relatively smooth overall structure. The core exhibits a bright, yellowish hue, suggesting an older stellar population. Fainter, bluish emissions extend outwards from the central region, hinting at the presence of younger stars and ongoing star formation. The galaxy has a slightly irregular shape, it is largely ellipsoidal. There are faint indications of potential tidal disturbances in the outer regions. The galaxy appears relatively isolated.
