The galaxy presents an elongated, cigar-shaped morphology. Its color distribution suggests a moderate amount of star formation activity. The central bulge exhibits a yellowish-orange hue, indicative of an older stellar population. Moving outwards from the core, the presence of a slightly bluish tint suggests more recent star formation in the outer regions. The galaxy appears generally smooth in structure, with no obvious signs of major disturbances or merging events. There may be a faint disk that lies at an angle relative to our point of view, causing the galaxy's elongated form.&#x20;
