The galaxy presents as a lenticular or elliptical type based on the image and supporting data. It exhibits a smooth, concentrated light profile with a high degree of central light concentration, appearing more rounded than elongated though not perfectly circular. There is no apparent structure in the form of spiral arms or a prominent disk. The color gradient suggests an older stellar population, displaying yellowish hues throughout the galaxy which might be indicative of a reduced rate of star formation. There is no evidence of any ongoing major mergers or tidal disturbances.
