The galaxy presents as a somewhat irregular, diffuse object with a moderate apparent size. Its overall shape is elongated, possibly indicative of a distorted or transitional morphology. The galaxy's light distribution appears uneven, with some regions exhibiting higher surface brightness than others. Within the galaxy, there is evidence of both smooth and more structured features. A smoother component is visible, possibly representing an older stellar population. Interspersed within the smoother component are regions that appear more clumpy or feature-rich, hinting at ongoing or recent star formation. These regions exhibit a bluer color, consistent with the presence of younger, hotter stars. There is a potential indication of minor tidal disturbances or interaction with another galaxy, though more data is needed to confirm this.
