The galaxy presents as a relatively smooth, elongated structure with a high degree of central concentration. The light distribution suggests an elliptical morphology or potentially a lenticular galaxy viewed edge-on. There's a hint of bluer light at one end of the major axis, possibly indicating a region of more recent star formation, though the dominant color is a more yellow-red hue, consistent with an older stellar population. Faint distortions or disturbances can be observed in the outer regions, potentially suggesting past or ongoing interactions with other galaxies or internal dynamical processes, though it could be nothing more than slight asymmetry in its overall shape. The galaxy appears to be relatively isolated, showing no clear signs of ongoing major merger activity in this image.