The galaxy presents an elongated, cigar-shaped morphology. A prominent central bulge exhibits a yellowish-white hue, indicative of an older stellar population. Extending outwards from the bulge, a faint disk-like structure is visible, exhibiting a bluer tinge suggesting the presence of younger stars and potential star formation regions. The disk appears somewhat disturbed or irregular, possibly hinting at past or ongoing interactions. The overall structure suggests an intermediate classification between a pure elliptical and a spiral galaxy, potentially a lenticular galaxy seen edge-on or a spiral with a dominant bulge and tightly wound arms. There is slight color variation implying potential difference in the stellar ages and composition across different regions. There may be some interactions happening given the slightly irregular structure.
