This galaxy exhibits an elongated, cigar-like morphology. The central region displays a concentrated luminosity, appearing smooth and yellowish-orange in color. A faint, bluish-white disk extends outwards from the central bulge, indicating the presence of a population of younger, hotter stars within the disk. There is a hint of possible disturbance in the disk, with a slight asymmetry observed along one edge, suggesting possible minor gravitational interaction with another galaxy in the past. Overall, the galaxy's smooth features dominate, implying the cessation of recent major merger activity. The object appears to be actively forming stars, though the specific star formation rate appears to be relatively low.
