The galaxy exhibits an elongated, cigar-shaped morphology. The light distribution appears relatively smooth, with a concentrated central bulge that transitions gradually into a more diffuse outer region. The color profile indicates a redder hue, especially concentrated in the center, suggesting an older stellar population. There is a hint of faint, extended features along the major axis that may be indicative of a tidal tail or stellar stream. The galaxy appears to be relatively undisturbed, with no signs of major ongoing mergers or strong tidal interactions. The estimated mass of the galaxy is high, suggesting a large number of stars. The star formation rate appears to be relatively low.
