The galaxy presents as a single, relatively smooth, and concentrated luminosity profile. There is an apparent radial color gradient, transitioning from a yellowish-white core to a redder outer region. The isophotes appear generally elliptical, although the image resolution limits a precise determination of ellipticity or the presence of any finer morphological features. The smooth appearance and color profile suggest a relatively evolved stellar population, with minimal evidence of recent or ongoing star formation. There is no visually detectable sign of spiral arms, bars, or tidal disturbances. The galaxy appears isolated, with no close companions or signs of interaction. The redshift indicates it is a distant object, consistent with the observed apparent magnitude and size.
