The galaxy presents as a roughly elliptical form with a concentrated central bulge. The light distribution appears relatively smooth with a fall off towards the edges, suggesting a minimal presence of defined spiral arms or intricate structures. Its overall morphology seems to lean towards a spheroid.

The color indices suggest that this is an older galaxy, with the g-r value greater than one. The object is slightly brighter in the r band than it is in the g band, and is brighter still in the z band.

There appears to be slight disturbance within the galaxy, possibly indicative of a minor interaction or merger event. The overall color profile is consistent with a passive, redder stellar population, punctuated by areas of localized bluer emission, particularly within what might be described as subtle ripples or asymmetries in the outer regions. These may indicate recent star formation triggered by the aforementioned interaction.
