The observed galaxy exhibits a primarily smooth morphology, with a discernible disk-like structure. Its overall shape is somewhat elongated, appearing between round and cigar-shaped. There is evidence of a possible minor disturbance within the galaxy, manifesting as slight irregularities in its outer regions. Specifically, a faint, blueish extension is visible on one side of the galaxy, possibly indicative of tidal interactions or recent star formation activity. The galaxy's central region appears more concentrated and exhibits a yellowish-orange hue. This may suggest an older stellar population. While the main body of the galaxy appears relatively undisturbed, the observed morphological features suggest a complex history possibly involving interactions with other galaxies.
