The galaxy appears as a somewhat irregular, diffuse structure. A central, brighter region can be discerned, possibly indicating a galactic bulge or a higher concentration of stars in the core. The outer regions exhibit a fainter, more spread-out distribution of light. There is evidence of spiral arm structures, though they are not well-defined. Patches of bluer light suggest ongoing star formation, interspersed with regions of older, redder stellar populations. The overall shape deviates from a perfect ellipse, possibly due to gravitational interactions. The galaxy shows signs of disturbance, evidenced by lumpy and diffuse features. A potential tidal tail or bridge may be present.
