This galaxy appears to be undergoing significant interaction or disturbance. Its overall morphology is irregular, lacking a clear spiral or elliptical structure. The central region exhibits a bright, concentrated core suggesting a high density of stars and potentially an active galactic nucleus. However, this brightness is not uniformly distributed, indicating either uneven dust obscuration or regions of heightened star formation.

Extending outwards from the core, we observe a diffuse, asymmetrical halo. There are notable features suggestive of tidal tails or disrupted arms, indicating gravitational interaction with another galaxy. Patches of bluer light are interspersed within the overall reddish hue, suggestive of ongoing star formation. The galaxy appears moderately distant.
