The galaxy presents as an elliptical or lenticular type, appearing predominantly smooth and featureless. Its overall shape is elongated, but significantly more rounded than a cigar shape. The central bulge region exhibits a yellowish hue, suggesting an older stellar population dominated by evolved stars. Progressing outwards, the galaxy's color gradually shifts towards a slightly bluer tint in the disk, potentially indicating the presence of some younger, hotter stars, but a lack of active star formation. There are no apparent spiral arms or dust lanes visible. No major mergers or major disturbances were found. The galaxy is quite large.
