The galaxy presents as a single, moderately concentrated object. It appears to be relatively smooth in texture with a slightly elongated shape. There is evidence of potential tidal disturbance in its form, suggesting the possibility of an ongoing or recent merger. The object is comprised of a complex distribution of light. The inner region is bluer than the outer edges, which shift more towards the yellow and red parts of the spectrum, suggesting a central concentration of younger, hotter stars surrounded by an older stellar population. A secondary, distinct, and redder component is also visible, possibly a satellite galaxy or a region of intense star formation.