The galaxy presents an elongated, somewhat irregular shape, suggesting it may be either an edge-on spiral or an elliptical galaxy undergoing some form of interaction. The central region appears brighter and more concentrated, possibly indicating a prominent galactic bulge. This bulge exhibits a yellowish hue, which could be indicative of an older stellar population. Fainter, bluer light extends outwards from the central region, suggesting the presence of younger, hotter stars in a disc-like structure. A faint, elongated structure to one side of the galaxy hints at a possible tidal tail or disruption due to a past or ongoing interaction. Overall, the galaxy displays a combination of features that could characterize it as an intermediate type between a classic elliptical and a more well-defined spiral galaxy.
