The galaxy presents as a luminous elliptical or lenticular structure. A bright, concentrated central bulge dominates the morphology, surrounded by a more diffuse and fainter halo. The halo exhibits an elongated shape, possibly hinting at a slight disk component or tidal interactions. The color gradient suggests a predominantly older stellar population within the bulge, trending towards a redder hue, while the outer regions show hints of bluer patches, possibly indicative of pockets of more recent, although minimal, star formation activity. There is a small possibility the galaxy may be interacting with another galaxy.
