The galaxy presents as a moderately inclined disk galaxy, roughly estimated to be around 7 kiloparsecs in diameter. It exhibits a slightly elongated morphology with a prominent central bulge. The bulge appears relatively smooth with a yellowish hue, suggesting an older stellar population. Faint, bluish spiral arm structures are visible, indicating regions of ongoing star formation, although these are not highly pronounced. There is little evidence of any major interaction or tidal disturbances. The overall light distribution is relatively smooth and symmetrical.