The galaxy presents an elongated morphology, suggesting it may be a disk galaxy viewed edge-on or a lenticular galaxy. The central bulge appears moderately bright and concentrated, exhibiting a yellowish hue, potentially indicating an older stellar population. The disk component shows a bluer color, particularly at the outer edges, which may signify ongoing star formation activity in these regions. The overall structure appears relatively smooth with minimal evidence of strong spiral arm features. The galaxy's light is significantly attenuated towards the edge of the disk, suggesting a substantial amount of dust. There is no obvious evidence of a strong interaction or recent merger. The galaxy appears to be a relatively isolated system in a settled state.
