The galaxy presents as a somewhat amorphous structure with a dominant central bulge. The core exhibits a yellowish-orange hue, indicative of an older stellar population. Fainter, diffuse extensions emanate from the central region, exhibiting a bluer color. These extensions suggest the presence of more recent star formation activity. The overall morphology leans towards a smooth, relatively featureless profile, yet there are subtle indications of potential disturbances or interactions, possibly minor tidal features, in the outer regions. The galaxy appears to be relatively isolated, with no clear evidence of a major ongoing merger, though subtle distortions suggest a possible past interaction.
