The galaxy presents a moderately inclined, elongated disk-like structure. The central region exhibits a concentrated, bright yellowish-white glow, suggesting an older stellar population likely residing in a bulge or nuclear region. Extending outwards from the center are fainter, somewhat diffuse regions, possibly indicative of a spiral disk. These regions appear bluer in color, hinting at the presence of younger, hotter stars and ongoing star formation. The overall shape appears to be cigar shaped, possibly with a minor disturbance.
