The galaxy appears as an elongated, diffuse structure, with an apparent bulge exhibiting a yellowish-orange hue, suggesting an older stellar population. Extending outwards from the central bulge is a more subtle disk component. This area shows hints of bluer light, possibly indicating the presence of younger, hotter stars, but the overall structure appears relatively smooth. There are suggestions of some irregularities in the disk with possible minor tidal features, indicating a possible past merger or ongoing interaction with another galaxy, though these are not distinct. Overall, the galaxy morphology appears to be somewhere between a spiral galaxy and an elliptical galaxy, with features of both. The galaxy exhibits a moderate redshift, indicating that we are looking at a relatively distant object. The apparent size of the galaxy, despite its distance, suggests it is a massive galaxy.
