The galaxy presents as a diffuse, elliptical-like object with a smooth light distribution. The color gradient suggests a population of older stars, with a redder hue towards the central region of the galaxy and a slightly bluer tint around the outskirts. This color distribution could be due to differential star formation history or dust obscuration. There is no apparent spiral structure or evidence of active star formation regions. The galaxy appears largely undisturbed, without any major tidal features or signs of ongoing merger activity. Its shape is somewhat elongated, tending toward a more rounded form, but with no signs of sharp edges or detailed features, likely a result of distance. Overall, this galaxy appears to be a relatively massive and quiescent system, consistent with an elliptical or lenticular type, with only minor disturbances or interactions.
