The galaxy presents as a relatively small, elongated structure. Its morphology suggests it is a spiral galaxy viewed at a high inclination angle, possibly approaching edge-on. A distinct central bulge is visible, although not sharply defined. The disk component of the galaxy exhibits some degree of irregularity, showing subtle hints of dust lanes or patchy star formation regions. The overall color appears predominantly reddish-yellow, implying an older stellar population and/or the presence of dust obscuring bluer light. Faint extensions or tidal features are not obviously discernible, indicating a lack of recent major merger events. The galaxy appears relatively isolated, with no obvious interacting companions. Some form of minor disturbance may be present within the disc.
