The galaxy presents a primarily smooth morphology with some discernible features suggesting disk-like structure. Its shape is elongated, appearing cigar-shaped rather than perfectly circular. The light distribution indicates a concentrated central bulge or core, emitting strongly in the yellow-red wavelengths. The galaxy exhibits a noticeable color gradient, transitioning from a redder hue near the core to a bluer tint towards the outer regions. This gradient potentially indicates the distribution of stellar populations, with older, redder stars concentrated in the core and younger, bluer stars more prevalent in the outer disk. There is a hint of possible tidal disturbance or interaction, evidenced by a slight asymmetry in the light distribution, perhaps indicating recent or ongoing minor merger activity. No prominent dust lanes are clearly visible, though some subtle obscuration effects could be present within the disk. Overall, the galaxy appears to be in a relatively quiescent state, showing low levels of star formation.
