The observed galaxy presents as a generally elliptical, though somewhat irregular, structure. A bright, concentrated central region dominates the galaxy's morphology, suggesting a prominent galactic nucleus. Extending outward from this bright core is a fainter, more diffuse halo. There appears to be a tail like structure that is extending from the bottom, suggesting possible tidal interactions. The color of the galaxy shifts from a brighter, blue white core to more of a yellow/orange hue in areas further from the center, suggesting a distribution of stellar populations with potentially older stars in the outer regions. Patches or disruptions seem to be visible, but are too indistinct to categorize.
