The galaxy presents as a spiral type, though the resolution limits definitive classification. Spiral arms are visible, exhibiting a fairly open morphology. These arms appear somewhat fragmented, hinting at regions of active star formation, albeit not strongly pronounced. There's a central bulge, which appears moderately sized, contributing significantly to the overall luminosity. The disk component shows a degree of patchiness, possibly due to dust obscuration or variations in stellar density. There is no clear evidence of a bar structure within the galaxy's central region. Additionally, there is no indication of any major merger events or significant tidal disturbances affecting the galaxy's morphology. Overall, the galaxy appears to be a relatively undisturbed spiral with moderate bulge dominance.
