The galaxy presents an elliptical morphology, appearing elongated in shape with a high degree of central concentration. The light profile exhibits a smooth distribution, indicative of an older stellar population. The galaxy appears largely featureless, lacking prominent spiral arms or dust lanes. The colour profile suggests a redder hue, possibly associated with evolved stars and low ongoing star formation activity. The ellipticity is quite high, close to that of a cigar. There are no signs of tidal disturbances or recent mergers.
