The galaxy presents a largely smooth morphology, with a notable absence of prominent spiral arms or a well-defined disk structure. The shape is neither perfectly circular nor elongated, appearing to be somewhere in between. There is no clear indication of a major merger event or significant tidal disturbances. Color gradients are visible; one region exhibits a bluer hue, which might indicate a population of younger, hotter stars or regions of ongoing star formation. Another region of the galaxy shows a distinct redder color, potentially indicating an older stellar population. The estimated size of the galaxy is approximately 5 kpc.
