The galaxy appears to be a disk galaxy, viewed at a near edge-on angle. A prominent central bulge is visible, exhibiting a reddish-orange hue, suggesting an older stellar population and minimal ongoing star formation in this region. A diffuse disk extends outwards from the bulge, displaying a bluer, more whitish color indicative of a younger stellar population and possibly active star formation. The disk appears relatively smooth, with some faint, irregular structures hinting at possible spiral arms or dust lanes. The overall shape suggests a classification somewhere between an elliptical galaxy and a spiral galaxy based on its structure and morphology. There might be evidence of a minor disturbance in the galaxy's morphology. The galaxy is not perfectly smooth or undisturbed, indicating a possibility of a past or ongoing interaction.
