The galaxy presents as an elongated, cigar-shaped structure. Its light profile appears relatively smooth, with no prominent spiral arms or distinct clumps of star formation readily apparent. The color distribution indicates a redder hue towards the central region of the galaxy, potentially signifying an older stellar population or higher dust concentration in that area. The outer regions appear bluer, suggesting the presence of younger stars, though this could be a result of less dust obscuration. There is a slight indication of minor disturbances in the galaxy's form, but overall, the main body of the galaxy appears relatively undisturbed and well-defined. No clear signs of a major merger or tidal interactions are immediately visible. 
