This galaxy appears to be a spiral galaxy, viewed at a highly inclined angle relative to our line of sight, close to edge-on. A prominent central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. Extending from the central bulge, a relatively faint disk can be discerned, with indications of dust lanes interspersed within the spiral arms. There is an overall reddish tint of the galaxy which suggests that it is distant. There appears to be some minor irregularity in the morphology, possibly indicative of gravitational interaction or minor disturbances. No major merger is apparent, although subtle tidal features might be present upon closer inspection. The galaxy is not entirely smooth, though also doesn't display strong distinct features. 
