The galaxy presents with a roughly elliptical morphology. There is a central bright core region, which likely indicates a significant concentration of stars or potentially an active galactic nucleus.

Surrounding the central core, there appears to be a fainter, more diffuse halo or disk-like structure, showing an assortment of colors. This extended region seems somewhat asymmetric. Indications of structural disturbance are present; there appear to be tidal features indicative of a possible minor merger or interaction.

There are also areas of intense star formation, possibly triggered by the merger event, with bright emissions in shorter wavelengths. The red and blue colors are distinctly separated. A few of the tidal features appear to be reddish in nature.
