The galaxy exhibits a notable disk-like morphology, observed at a near edge-on orientation. A prominent bulge is visible, displaying a yellowish hue, indicative of an older stellar population. The disk component presents a bluer color, suggesting ongoing star formation. A considerable amount of disturbance is observed in the disk, possibly indicative of a past or ongoing merger event. The lower region shows a more diffuse, somewhat detached component, distinct from the main disk structure. This feature may be a tidal tail or a remnant of an interaction with another galaxy. There is a slight asymmetry to the overall structure of the galaxy, further supporting the likelihood of a gravitational interaction.
