The galaxy appears as a slightly irregular elliptical or lenticular type, displaying a dominant, centrally concentrated bulge. The core region exhibits a bright, yellowish hue, suggesting a population of older stars and potentially significant dust content. Extending outwards from the core, there is a fainter, diffuse disk component, with a hint of spiral structure, but the arms are not well-defined. Patches of bluer light may indicate regions of recent star formation, though these are not particularly prominent. There is a very slight asymmetry in the galaxy's overall structure, with one side appearing somewhat more extended than the other, which may suggest minor tidal disturbances or past merger events.
