The galaxy presents as an elongated structure, appearing somewhat cigar-shaped in overall form. It exhibits a generally smooth texture, though some features are discernible. One end of the galaxy has a distinct bulge or condensation of light, possibly indicating a central galactic nucleus or a region of heightened stellar density. The luminosity appears brighter in the G, R and Z bands, with a slightly increasing luminosity towards the redder bands.

A fainter arm-like extension or tidal feature is noticeable emanating from the opposite end of the galaxy, suggesting a possible past interaction or disturbance. This may indicate a minor merger event. There is a possibility of minor dust lanes present. The overall color is biased towards the bluer end of the spectrum, indicative of ongoing star formation or a younger stellar population. There are some areas of redder colors that are scattered within the bluer regions, likely marking regions of relatively more dust and possibly older stars.
