The galaxy appears as a centrally concentrated object, likely an elliptical or lenticular galaxy given the overall smooth, featureless morphology. It exhibits a strong central bulge with a gradual decrease in luminosity outwards, indicating a relatively high concentration of stars in the core. There are subtle color gradients across the galaxy, with the central region exhibiting a yellowish hue that transitions to slightly bluer tones towards the outer regions. This suggests the presence of a relatively older stellar population in the core with potentially some ongoing or recent star formation activity in the outer regions. The galaxy seems generally undisturbed with no signs of a major ongoing merger, although subtle asymmetries in the outer regions might indicate minor tidal interactions in the past or a possible minor merger event. The galaxy appears to be relatively massive, with its high luminosity and size indicative of a galaxy that is more massive than an average galaxy in the local universe.
