The galaxy presents as a somewhat elliptical structure, exhibiting a notable degree of smoothness in its overall form. There's a hint of a more defined central bulge region.  The color profile indicates a mixture of stellar populations, with bluer hues present. The galaxy appears to be undergoing some form of interaction, possibly a merger or tidal disruption, showing morphological asymmetry with potential distortion in its shape and the presence of features indicative of ongoing or past interactions. The overall impression is of a galaxy in a state of dynamic evolution, likely influencing its star formation rate.
