The galaxy appears to be undergoing significant interaction, possibly a merger or a close tidal interaction with another galaxy outside of the field of view. One component presents a smooth, somewhat elliptical morphology with a yellowish hue, suggesting an older stellar population. Connected to this is a distinct, elongated feature exhibiting a bluer color, indicative of ongoing or recent star formation. This blue region appears less organized and potentially tidally stretched or disrupted, forming an arm-like structure extending away from the main body. There are traces of disturbed morphology within both components. This galaxy presents a relatively low rate of star formation. The overall shape is somewhat irregular, and the lack of clear spiral arms further suggests a system undergoing dynamic changes due to gravitational interactions.
