The galaxy presents as a smooth, centrally concentrated object. Its overall shape is elongated, appearing somewhat cigar-shaped rather than perfectly circular. The light distribution suggests a dominant spheroid component, likely an elliptical galaxy. The core exhibits a yellow-orange hue, suggestive of an older stellar population with less ongoing star formation. Fainter, bluer fringes are very subtly visible at the edges, potentially indicating regions of more recent, but still limited, star formation. There is no clear evidence of spiral arms, bars, or significant dust lanes. The galaxy does not show strong indications of any major ongoing mergers or disturbances to its morphology, however a very slight tidal tail may be forming on the edge, or it could be a redder and larger artifact.
