The galaxy presents as a moderately bright, elongated structure with a cigar-like morphology. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population. Progressing outwards from the center, a subtle shift towards bluer tones is observed, particularly noticeable at the polar regions. The morphological classification appears to lean towards a smooth structure with some suggestion of features along the main axis. There is no obvious indication of strong tidal disturbances or ongoing major mergers, although some subtle asymmetries are present. A small object near the edge has a blue-shifted appearance, suggestive of a possible star forming region or a smaller interacting galaxy. The galaxy has an estimated stellar mass of approximately 10^9.9 solar masses. Star formation is present, with an inferred star formation rate that places it within the star-forming category.
