The galaxy presents as a moderately distant, relatively small, elongated object. Its overall shape appears to be a flattened spheroid, cigar-shaped, suggesting an elliptical morphology or a spiral galaxy viewed at a steep inclination. The galaxy exhibits a smooth texture with no distinct spiral arm structures visible at this resolution. It displays a subtle color gradient, being slightly bluer on the edges which may hint at potential star formation activity. There is no distinct central bulge that can be determined, due to the inclination. No signs of major mergers or strong tidal disturbances can be determined. Further observations are required to confirm the morphological type and star formation rates.
