The galaxy appears as a relatively faint, elongated object. Its disk is oriented edge-on, presenting a needle-like profile. Some slight warping may be present, though not overtly disrupted. The galaxy's color index indicates that it is likely a relatively massive galaxy. The image resolution limits a more detailed analysis of internal structures, such as dust lanes or spiral arm features. There may be signs of low-level interaction, perhaps due to tidal forces or a possible minor merger. Overall, the galaxy presents itself as a substantial, late-type system viewed along its equatorial plane, potentially undergoing some form of minor interaction.
